Evermore

I'd like to pack this
And take you to the stars
We'll eat in fancy restaurants
And drive in fancy cars
We've tried our luck, we made a buck
So lean back have some fun

Oh yes my love
But first just this last one
We stood on these cliffs on a starless night
I held your hand in mine
So stand by me with all your heart
I'll need you by my side

Oh the river is cold and black
And the bottom is a long way down
Another one going underground
Why can't we cut the ropes
And let that poor fool go

Don't you go getting weak on me
Not when I need you so
Don't lose your step
Now we're almost there
Go wash your face and comb your hair
So trust me now, believe in me
Forever more your love you have pledged to me

We'll stay at home and call this day our own
Listen to a record, watch a candle burn
I'm feeling kinda drowsy
There's blood on the floor
When I'm gone you still will have
My love for evermore

Cafe Racer History

It is perhaps the most influential motorcycle movement the world has ever seen. Born in the streets of England in the 1950s, its culture still thrives around the globe. There will never be another motorcycle—or rider—quite like it. And yet, most of us have never heard of the café racer.

The café racer is both man and machine. With its Spartan appearance and aggressive styling, the café racer is one of the most distinctive and revered motorcycles in the world. Their impact on the motorcycle industry includes legendary high-performance motorcycles like Triumph’s Bonneville, Honda’s CB-750, and Kawasaki’s Z-1. Without the original café racers tuning and designing their ordinary street bikes for power and handling, manufacturers may never have designed the modern sportbike.

The café racer movement may have been born in London in the 1950s, but it has developed into a subculture encompassing a desire for speed, a love of rock and roll, and ultimately an enduring love for a motorcycle that’s being revived worldwide.The human side of the café racer was a perfect match for this type of motorcycle. The riders of these machines were young, and they wanted to go fast. The goal of many of the café racers during the 50s was the ability to hit a hundred miles an hour, better known as “the ton.” Author and journalist Mike Seate has been following the café racer for two decades.

“The term café racer came from what’s actually a derisive term used to describe kids who hung out in cafés and raced fast. They would hang out in transport cafés and wait until somebody else came by on a fast bike and challenged them for a race, and they all rushed outside to see who gets up the road the fastest. When they get back to the cafés, which were often occupied by long distance truck drivers, the truck drivers would laugh and say, ‘You’re not a real racer, you’re not Barry Sheen, you’re just a café racer! And the kids thought, ‘Well you’re damn right I’m a café racer!’ So they would race to the next café, and then to the next one as fast as they could, and the name stuck; they embraced it despite the fact that it was a derisive term,” he said.

One of the birthplaces of the café racer was London’s Ace Café. The Ace was one of many cafés that provided a gathering place for teenagers and their motorcycles in the 1950s and 60s. Many, like the Busy Bee and Café Rising Sun have succumbed to the wrecking ball, while others, such as Jack’s Hill and Squires Coffee Bar have survived, hosting annual Ton-Up reunions each year. Avid motorcyclist Mark Wilsmore, who reopened the Ace Café to its former glory in 1994, says that rock and roll helped spark the subculture known as “ The Café Racing.”

“These kids over here, they have been the generation—rock and roll generation—they went out and bought the fastest vehicle they could afford, which over here was a motorbike. In the States, that was a car, and you had your hot rod culture come directly out of Elvis Presley and that lot, but over here, we had a similar sort of thing, but all based around motorbikes because of our different income levels.  And the other great attraction of cafés, and I suspect diners in the states at that time, was the jukebox. And certainly in this country, when rock and roll first came around in the mid-50s you could only hear rock and roll on the jukebox. There was no radio stations playing it, no clubs playing it, so this new music of youngsters mixed with having their own vehicles and their own identity, um, along comes this Ton-Up boy and his bike, the café racer, it was invariably—the racing would be from one café to another,” he said. The hunger to make their ordinary streetbikes go faster and resemble the machines ridden by British racing heroes like Mike Hailwood and Geoff Duke was all part of the café racer’s character. Doing the “Ton,” or hitting a hundred miles-an-hour, became a badge of honor—weather you made it back…or not.

Riders from those days say attempts at reaching the “Ton” on your average 650cc parallel twin were dodgy affairs at best. Riders could consider themselves very, very lucky to reach it as their engines had to be tuned well, but even the best engines could out-perform the skinny, bias-ply tires and meager drum brakes of mid-century design. Road surfaces were not what they are today, with everything from poor road lighting to axle grease from cars and trucks making each corner a potential deathtrap. Trial and plenty of error was the order of the day and the Rockers, experimenting with countless performance modifications, came to create motorcycles that are still respected by go-fast aficionados. Brave? Crazy? Brilliant visionaries? Addicted to kicks? The Rockers were, and are, all of the above, which is why the Café Racer culture still lives not only in the streets on London, but across the globe.  Enthusiasts of all ages are once again building custom high-performance motorcycles out of their garages, machines that continue the tradition of the café racer.  Join us for Discovery HD Theater’s “Café Racer TV” as we explore this rich history and the quest to “Do The Ton.”

^_^

This evening the atmosphere is so tense, for some reason I have never been so scared baseball, inside the room, I can not get to sleep awake, looked around the room that are red, occasionally peeking from pejaman eyes, I seemed to know if there will be approached. Ah, maybe this is just a feeling I wrote, occasionally smiled and said to myself "Sleeping yuk, Gofar", clearing diary plus a small padlock which is next to the head, kissing teddy bear, interesting quilt Kero Kero Keroppi and now it's time to sleep. Hose five minutes passed, the sound of a loud knock on the door, so loud! "TOK TOK TOK! TOK TOK TOK! ", Snapped this self open eyes, the sweat condenses on the forehead, began a rhythmic heartbeat Dubstep, woke up from the bed and peered toward the door while bebisik softly," Who the hell? Aa .. is this a ghost or a human being? "

With slow steps uncertain dragging on the floor, the courage to open the door, knock on the door louder voice and repeated, over and over and over and over again! Tersodor wrist toward the doorknob, shaking finally I pull the door handle, "BRUAKK!" Oohh, apparently looking for bu Djoko next door neighbor would borrow a thermos of ice, one of the house turned out. Fiuhh there is no aja. With that incident made me baseball mood to sleep, finally, I wear shorts and T-shirts Mambo Grifone side lines hanging in the closet and decided to go to the shop in search of food, it turns out the incident was quite draining and raised hunger.

Arriving at tavern eat close to home, it appears there was a little tension there, a grumpy mustachioed champion, pound the table shouting "I'M THE MOST AWFUL!" And the waiter was bringing food while gemeteran. Because the males took part in the situation, I was reversing direction back toward the house. At home my car heats, decided to spend the night at the residence of friends taulan. Increasingly felt late night and cold, any desirewant to continue together to listen to a song Java Jive accompany my journey. Arriving on the highway, look beautiful girl the toll gate keeper, judging by her name tag, it turns out he was named Elma Theana and somehow this lip automatically saying "Xoncenya mannnnnna?" Thrusting a toll dues money, grotesque.

With speeds ala Knight Rider Michael Knight, the car speeding on the highway, do not feel the needle car dashboard showed gasoline was dying, I stop by the gas station on the highway. When I got there I came down from the car to buy Premix or Super TT fuming annoyed "Ah this car is extravagant!", Looks a father to hear what I then walked, smiled and said: "AMPA Empa tens of thousands" with the accent Bali pointing black car, whatever that means.

Okay, time to move on. A few meters left the gas station suddenly the car engine off, distarter baseball flames, strike brothers! Then the rain was pouring down, whether there is anything with me this evening. Waited in the car while occasionally trying the starter again but to no avail, I finally gave up, leaning head on the headrest, closed his eyes while chewing crunchy Kayane cruncy and Butternut Collins I like all like the taste of pure material patents. Soon there was a knock windshield, visible figure of a woman soaking rain, I open the windshield, "What are you doing here?" Said the woman who turned out to be a former me, "The car I strike" said I, "Yauda left his car here aja , later telephone tow truck, now I anther you wrote it to your house? "asked the former. I also affirm the offer and went to his car, candy given to him, "You better deh" I whispered into her ear, and then we hugged tightly as if he did not want to be separated, in my heart said, "Cold-cold soft".

At home I waved good-hearted ex who had willingly drove up to the house, soaking wet and then I went into the house, took a towel and a bath, wash with shampoo scent of fruit while singing "Dee dee it shampoku, I shower every dee jitak "to appease hearts lara. Turns shampooing once is not enough, I also repeat wash hair with shampoo Johnson's Baby with murmuring the song composed by Dan Hill - Sometimes When We Touch, "There is a language of love mlalui your touch, and I know language of love ~". bathing all completed and it has been a little quiet heart, to be more calm again I took a bottle of powder and sow in my body by chanting the song "Loose skin powder blushes Rodeka your family Ro De Ka".

What a night, a night which was incredible. Genesis truly unexpected, this self silent, staring at the mirror a few minutes then smiled and whispered in front of the mirror "Your hair, like Anjasmara", mantra pep to sleep. Heading to bed again, lay down to its original position, turn off the lights as if light "glare MEN!" And it is time to sleep. So the ladies and gentlemen of this story has a happy ending endings. Moral message implicit in this story is, if there are people who pretended to know, say

This sentence in front of her face: "Ah Teori!"


-pergi jauh-

Global Warming

     Global warming, the phenomenon of increasing average air temperatures near the surface of Earth over the past one to two centuries. Climate scientists have since the mid-20th century gathered detailed observations of various weather phenomena (such as temperatures, precipitation, and storms) and of related influences on climate (such as ocean currents and the atmosphere’s chemical composition). These data indicate that Earth’s climate has changed over almost every conceivable timescale since the beginning of geologic time and that the influence of human activities since at least the beginning of the Industrial Revolution has been deeply woven into the very fabric of climate change.

     Giving voice to a growing conviction of most of the scientific community, the Intergovernmental Panel on Climate Change (IPCC) was formed in 1988 by the World Meteorological Organization (WMO) and the United Nations Environment Program (UNEP). In 2013 the IPCC reported that the interval between 1880 and 2012 saw an increase in global average surface temperature of approximately 0.9 °C (1.5 °F). The increase is closer to 1.1 °C (2.0 °F) when measured relative to the preindustrial (i.e., 1750–1800) mean temperature.

The IPCC stated that most of the warming observed over the second half of the 20th century could be attributed to human activities. It predicted that by the end of the 21st century the global mean surface temperature would increase by 0.3 to 4.8 °C (0.5 to 8.6 °F) relative to the 1986–2005 average. The predicted rise in temperature was based on a range of possible scenarios that accounted for future greenhouse gas emissions and mitigation (severity reduction) measures and on uncertainties in the model projections. Some of the main uncertainties include the precise role of feedback processes and the impacts of industrial pollutants known as aerosols which may offset some warming.

     Many climate scientists agree that significant societal, economic, and ecological damage would result if global average temperatures rose by more than 2 °C (3.6 °F) in such a short time. Such damage would include increased extinction of many plant and animal species, shifts in patterns of agriculture, and rising sea levels. The IPCC reported that the global average sea level rose by some 19–21 cm (7.5–8.3 inches) between 1901 and 2010 and that sea levels rose faster in the second half of the 20th century than in the first half. It also predicted, again depending on a wide range of scenarios, that by the end of the 21st century the global average sea level could rise by another 26–82 cm (10.2–32.3 inches) relative to the 1986–2005 average and that a rise of well over 1 metre (3 feet) could not be ruled out.

     The scenarios referred to above depend mainly on future concentrations of certain trace gases, called greenhouse gases, that have been injected into the lower atmosphere in increasing amounts through the burning of fossil fuels for industry, transportation, and residential uses. Modern global warming is the result of an increase in magnitude of the so-called greenhouse effect, a warming of Earth’s surface and lower atmosphere caused by the presence of water vapour, carbon dioxide, methane, nitrous oxides, and other greenhouse gases. In 2014 the IPCC reported that concentrations of carbon dioxide, methane, and nitrous oxides in the atmosphere surpassed those found in ice cores dating back 800,000 years. Of all these gases, carbon dioxide is the most important, both for its role in the greenhouse effect and for its role in the human economy. It has been estimated that, at the beginning of the industrial age in the mid-18th century, carbon dioxide concentrations in the atmosphere were roughly 280 parts per million (ppm). By the middle of 2014, carbon dioxide concentrations had briefly reached 400 ppm, and, if fossil fuels continue to be burned at current rates, they are projected to reach 560 ppm by the mid-21st century—essentially, a doubling of carbon dioxide concentrations in 300 years.

     A vigorous debate is in progress over the extent and seriousness of rising surface temperatures, the effects of past and future warming on human life, and the need for action to reduce future warming and deal with its consequences. This article provides an overview of the scientific background and public policy debate related to the subject of global warming. It considers the causes of rising near-surface air temperatures, the influencing factors, the process of climate research and forecasting, the possible ecological and social impacts of rising temperatures, and the public policy developments since the mid-20th century. For a detailed description of Earth’s climate, its processes, and the responses of living things to its changing nature, see climate. For additional background on how Earth’s climate has changed throughout geologic time, see climatic variation and change. For a full description of Earth’s gaseous envelope, within which climate change and global warming occur, see atmosphere.

Climatic variation since the last glaciation

     Global warming is related to the more general phenomenon of climate change, which refers to changes in the totality of attributes that define climate. In addition to changes in air temperature, climate change involves changes to precipitation patterns, winds, ocean currents, and other measures of Earth’s climate. Normally, climate change can be viewed as the combination of various natural forces occurring over diverse timescales. Since the advent of human civilization, climate change has involved an “anthropogenic,” or exclusively human-caused, element, and this anthropogenic element has become more important in the industrial period of the past two centuries. The term global warming is used specifically to refer to any warming of near-surface air during the past two centuries that can be traced to anthropogenic causes.

     To define the concepts of global warming and climate change properly, it is first necessary to recognize that the climate of Earth has varied across many timescales, ranging from an individual human life span to billions of years. This variable climate history is typically classified in terms of “regimes” or “epochs.” For instance, the Pleistocene glacial epoch (about 2,600,000 to 11,700 years ago) was marked by substantial variations in the global extent of glaciers and ice sheets. These variations took place on timescales of tens to hundreds of millennia and were driven by changes in the distribution of solar radiation across Earth’s surface. The distribution of solar radiation is known as the insolation pattern, and it is strongly affected by the geometry of Earth’s orbit around the Sun and by the orientation, or tilt, of Earth’s axis relative to the direct rays of the Sun.

     Worldwide, the most recent glacial period, or ice age, culminated about 21,000 years ago in what is often called the Last Glacial Maximum. During this time, continental ice sheets extended well into the middle latitude regions of Europe and North America, reaching as far south as present-day London and New York City. Global annual mean temperature appears to have been about 4–5 °C (7–9 °F) colder than in the mid-20th century. It is important to remember that these figures are a global average. In fact, during the height of this last ice age, Earth’s climate was characterized by greater cooling at higher latitudes (that is, toward the poles) and relatively little cooling over large parts of the tropical oceans (near the Equator). This glacial interval terminated abruptly about 11,700 years ago and was followed by the subsequent relatively ice-free period known as the Holocene Epoch. The modern period of Earth’s history is conventionally defined as residing within the Holocene. However, some scientists have argued that the Holocene Epoch terminated in the relatively recent past and that Earth currently resides in a climatic interval that could justly be called the Anthropocene Epoch—that is, a period during which humans have exerted a dominant influence over climate.

     Though less dramatic than the climate changes that occurred during the Pleistocene Epoch, significant variations in global climate have nonetheless taken place over the course of the Holocene. During the early Holocene, roughly 9,000 years ago, atmospheric circulation and precipitation patterns appear to have been substantially different from those of today. For example, there is evidence for relatively wet conditions in what is now the Sahara Desert. The change from one climatic regime to another was caused by only modest changes in the pattern of insolation within the Holocene interval as well as the interaction of these patterns with large-scale climate phenomena such as monsoons and El Niño/Southern Oscillation (ENSO).

     During the middle Holocene, some 5,000–7,000 years ago, conditions appear to have been relatively warm—indeed, perhaps warmer than today in some parts of the world and during certain seasons. For this reason, this interval is sometimes referred to as the Mid-Holocene Climatic Optimum. The relative warmth of average near-surface air temperatures at this time, however, is somewhat unclear. Changes in the pattern of insolation favoured warmer summers at higher latitudes in the Northern Hemisphere, but these changes also produced cooler winters in the Northern Hemisphere and relatively cool conditions year-round in the tropics. Any overall hemispheric or global mean temperature changes thus reflected a balance between competing seasonal and regional changes. In fact, recent theoretical climate model studies suggest that global mean temperatures during the middle Holocene were probably 0.2–0.3 °C (0.4–0.5 °F) colder than average late 20th-century conditions.

     Over subsequent millennia, conditions appear to have cooled relative to middle Holocene levels. This period has sometimes been referred to as the “Neoglacial.” In the middle latitudes this cooling trend was associated with intermittent periods of advancing and retreating mountain glaciers reminiscent of (though far more modest than) the more substantial advance and retreat of the major continental ice sheets of the Pleistocene climate epoch.

Causes of global warming

The greenhouse effect

     The average surface temperature of Earth is maintained by a balance of various forms of solar and terrestrial radiation. Solar radiation is often called “shortwave” radiation because the frequencies of the radiation are relatively high and the wavelengths relatively short—close to the visible portion of the electromagnetic spectrum. Terrestrial radiation, on the other hand, is often called “longwave” radiation because the frequencies are relatively low and the wavelengths relatively long—somewhere in the infrared part of the spectrum. Downward-moving solar energy is typically measured in watts per square metre. The energy of the total incoming solar radiation at the top of Earth’s atmosphere (the so-called “solar constant”) amounts roughly to 1,366 watts per square metre annually. Adjusting for the fact that only one-half of the planet’s surface receives solar radiation at any given time, the average surface insolation is 342 watts per square metre annually.

     The amount of solar radiation absorbed by Earth’s surface is only a small fraction of the total solar radiation entering the atmosphere. For every 100 units of incoming solar radiation, roughly 30 units are reflected back to space by either clouds, the atmosphere, or reflective regions of Earth’s surface. This reflective capacity is referred to as Earth’s planetary albedo, and it need not remain fixed over time, since the spatial extent and distribution of reflective formations, such as clouds and ice cover, can change. The 70 units of solar radiation that are not reflected may be absorbed by the atmosphere, clouds, or the surface. In the absence of further complications, in order to maintain thermodynamic equilibrium, Earth’s surface and atmosphere must radiate these same 70 units back to space. Earth’s surface temperature (and that of the lower layer of the atmosphere essentially in contact with the surface) is tied to the magnitude of this emission of outgoing radiation according to the Stefan-Boltzmann law.

     Earth’s energy budget is further complicated by the greenhouse effect. Trace gases with certain chemical properties—the so-called greenhouse gases, mainly carbon dioxide (CO2), methane (CH4), and nitrous oxide (N2O)—absorb some of the infrared radiation produced by Earth’s surface. Because of this absorption, some fraction of the original 70 units does not directly escape to space. Because greenhouse gases emit the same amount of radiation they absorb and because this radiation is emitted equally in all directions (that is, as much downward as upward), the net effect of absorption by greenhouse gases is to increase the total amount of radiation emitted downward toward Earth’s surface and lower atmosphere. To maintain equilibrium, Earth’s surface and lower atmosphere must emit more radiation than the original 70 units. Consequently, the surface temperature must be higher. This process is not quite the same as that which governs a true greenhouse, but the end effect is similar. The presence of greenhouse gases in the atmosphere leads to a warming of the surface and lower part of the atmosphere (and a cooling higher up in the atmosphere) relative to what would be expected in the absence of greenhouse gases.

     It is essential to distinguish the “natural,” or background, greenhouse effect from the “enhanced” greenhouse effect associated with human activity. The natural greenhouse effect is associated with surface warming properties of natural constituents of Earth’s atmosphere, especially water vapour, carbon dioxide, and methane. The existence of this effect is accepted by all scientists. Indeed, in its absence, Earth’s average temperature would be approximately 33 °C (59 °F) colder than today, and Earth would be a frozen and likely uninhabitable planet. What has been subject to controversy is the so-called enhanced greenhouse effect, which is associated with increased concentrations of greenhouse gases caused by human activity. In particular, the burning of fossil fuels raises the concentrations of the major greenhouse gases in the atmosphere, and these higher concentrations have the potential to warm the atmosphere by several degrees

Radiative forcing

     In light of the discussion above of the greenhouse effect, it is apparent that the temperature of Earth’s surface and lower atmosphere may be modified in three ways: (1) through a net increase in the solar radiation entering at the top of Earth’s atmosphere, (2) through a change in the fraction of the radiation reaching the surface, and (3) through a change in the concentration of greenhouse gases in the atmosphere. In each case the changes can be thought of in terms of “radiative forcing.” As defined by the IPCC, radiative forcing is a measure of the influence a given climatic factor has on the amount of downward-directed radiant energy impinging upon Earth’s surface. Climatic factors are divided between those caused primarily by human activity (such as greenhouse gas emissions and aerosol emissions) and those caused by natural forces (such as solar irradiance); then, for each factor, so-called forcing values are calculated for the time period between 1750 and the present day. “Positive forcing” is exerted by climatic factors that contribute to the warming of Earth’s surface, whereas “negative forcing” is exerted by factors that cool Earth’s surface.

On average, about 342 watts of solar radiation strike each square metre of Earth’s surface per year, and this quantity can in turn be related to a rise or fall in Earth’s surface temperature. Temperatures at the surface may also rise or fall through a change in the distribution of terrestrial radiation (that is, radiation emitted by Earth) within the atmosphere. In some cases, radiative forcing has a natural origin, such as during explosive eruptions from volcanoes where vented gases and ash block some portion of solar radiation from the surface. In other cases, radiative forcing has an anthropogenic, or exclusively human, origin. For example, anthropogenic increases in carbon dioxide, methane, and nitrous oxide are estimated to account for 2.3 watts per square metre of positive radiative forcing. When all values of positive and negative radiative forcing are taken together and all interactions between climatic factors are accounted for, the total net increase in surface radiation due to human activities since the beginning of the Industrial Revolution is 1.6 watts per square metre.

The influences of human activity on climate

     Human activity has influenced global surface temperatures by changing the radiative balance governing the Earth on various timescales and at varying spatial scales. The most profound and well-known anthropogenic influence is the elevation of concentrations of greenhouse gases in the atmosphere. Humans also influence climate by changing the concentrations of aerosols and ozone and by modifying the land cover of Earth’s surface.

Greenhouse gases

     As discussed above, greenhouse gases warm Earth’s surface by increasing the net downward longwave radiation reaching the surface. The relationship between atmospheric concentration of greenhouse gases and the associated positive radiative forcing of the surface is different for each gas. A complicated relationship exists between the chemical properties of each greenhouse gas and the relative amount of longwave radiation that each can absorb. What follows is a discussion of the radiative behaviour of each major greenhouse gas

http://www.britannica.com 

Tugas Softskill bahasa inggris bisnis 2

1. What is relative clause ! explain and find a passage then you determine its relative clause.

Relative clause is part of the sentences (clause) which specifies the person or thing that precedes it. The term relative clauses with adjective clause. Mentioned adjective clause because he explains things or people that preceded them. Mentioned relative clause because connect (me-Relate) the thing or person is the phrase on the back. Relative clauses begin with the preposisition who, whom, whose, which, that, with, the following functions :

Who : describe the person as a subject

Whom : present state of the object (replace me, you, us, him, her, them, it)

Whose : describing people as owners (replacing my, your, our, his, her, their, its)

Which : describing things as subject or object

That : explains a good person or thing as the subject or object

Example :

·         He is the man who works hard to support their daily needs.

·         The woman whom you saw last night is my sister.

·         The man, whose car is antique, works as a lecturer.

·         Mueeza, which is very faithful, is my cat

·         It is the car that I have dreamed for many years ago.

2. What is conditional sentences ! how many types of conditional sentences are there ? make examples for each type !

Conditional Sentence is a sentence that contains the assumption is often called a conditional sentence where an event will be fulfilled if the condition is met. In a sentence of conditional sentences, there are two clauses, namely: main clause and the if clause.

The types of conditional sentence:       3

Type I (future)

This first type of conditional sentences refer to future events (future) so the fact or facts of his statement is still a possibility that may happen or may not happen. The first type of conditional pattern is as follows:

If + simple present, future tense

if + Simple Present, will-Future

examples :

·         If you give me money, I will help you.

·         If you help me, I will Give you money

·         If you leave your sister alone, she will miss you.

·         If our team win the match, we will be very happy.

·         If joni camps, he will build a campfire

Type II (present)

Sentence type II modality is a modality for the present sentence kaliamat which is contrary to the events occurring in the present (present). So the facts in the present tense.b. Type II (present). Sentence type II modality is a modality for the present sentence kaliamat which is contrary to the events occurring in the present (present). So the facts in the present tense.

If + simple past tense, past future tense

If + Simple Past, main clause with Conditional I (= would + Infinitive)

examples :

·         If I were you, I would be very angry

·         If I were superman, I would fly to the moon

·         If I married Anna, I would be very happy

·         If I were an entrepreneur, I would  get money easily

·         If you followed my instruction, you would be safe.

Type III (past)

Type III conditional sentence is a sentence modality for the past where the sentence is contrary to the reality that happened in the past (past). So should the fact that in the past tense.

If + past perfect tense, past perfect future

If + Past Perfect, main clause with Conditional II

examples :

·         If grandfather had been immediately taken to the hospital, he would havebeen saved.

·         I would have sent her an invitation if I had found her address.

·         If I had found her address, I would have sent her an invitation.

·         If berry had Realize how hurt it was for me, He would have said sorry.

If Jono had studied hard, he would have passed the exam.