Solar Space Weather

On the other hand, the geomagnetic storms have been intensified and enhanced in their frequency as magnetic fields of coronal mass ejections indulges with that of the earth that causes change of direction and leave more radiation and magnetic energy into the environment of the planet earth. Solar Hemispheric Observatory and Solar

The foremost differentiation between solar flares and coronal mass ejections (CMEs) is the scale on which they transpire. Solar flares are rather little and local, occuring in the low solar atmosphere, near sunspots, where magnetic field lines are concentrated. CMEs on the other hand are huge. They can even be bigger than the sun itself!

3. Solar Flares: these are ejections of large volumes of gas. They can sometimes head our way causing radio interference and auroras.

However, this has not happened and it’s starting to make secular scientist themselves admit that our sun is special and unique in design, because it does not emit these monster super flares like the ones produced by Proxima Centauri. The question is, could our sun send out such a flare powerful enough to even melt the ice on Jupiter’s moon’s, destroy earth’s ozone layer and even obliterate all our satellites? Well the answer is yes. Scientist have studied other sun like stars in our galaxy and discovered that they produce these super flares about once a century. But, they have no explanations as to why our sun does not produce such solar

Despite the amounts of incoming radiation, very little actually reaches the Earth’s surface. One layer of protection the Earth provides is in the form of a magnetic field that deflects charged particles from reaching the Earth’s surface. This magnetic field is generated by a combination of the liquids within the Earth’s core and the interplanetary magnetic field generated by the Sun. This field reaches out thousands of miles from Earth, so when solar wind travels through space and encounters Earth’s

In the year 2065, climate change on Earth has spiraled out of control and nations are now fighting for new real estate in space to begin colonization. Mars had been a likely candidate for many years now and was becoming a massive fighting ground for numerous nations. However, it’s arid landscape and small size made it a questionable choice to some. More adventurous and risk-taking politicians urged their researchers to aim for Pluto or planets outside of our solar system. Feeling modern technology was not yet ready for such long distance travel, the United States has chosen to look toward the asteroid belt. As they are setting off, researchers will monitor sunspots to help forecast the behavior of the sun and predict coronal mass ejections (CMEs). Solar-powered sails will make use of solar wind for the early journey after leaving Earth. Radioisotope thermoelectric

Sunspots aren’t that complicated they’re really just dark spots on the sun’s surface. Now these sunspots have a strong magnetic field and always in motion. The sunspots take around 27 days or so to rotate, but we can only see, so much from the Earth’s surface, but for now 27 days would be our best answer. Now you probably haven’t heard about solar maximum or minimum, but they are also related to the topic of sunspots. They really just mean if their is no sunspots, solar minimum, and if their is the most we could possibly see, solar maximum, and both would be seen from earth, not space. Their is this thing where the sun envelops the Earth with energy, such as light and these elecrtically charged magnetic fields, or particles. This is what people call solar weather and after the earth is bathed with the forms of energy, their is only an effect that affects us durring an auroral event. If solar weather hits during an auroral event power grids may get

Solarwinds, a “stream of charged particles from the sun’s upper part of the atmosphere, called Corona”. They said to be made out of hydrogens protons and electrons. Also having a traces of atomic nuclei and alpha particles. The Astrophysicist who first discovered this amazing thing, formerly known as Eugene Parker. It wasn't until 1958 when notice,“stiff

--On approach to mars, a solar superstorm erupts. A solar flare is a quick release of energy from the Sun’s surface. Flares are classified logarithmically, like the Richter scale, with the highest being X class. An X10 flare would be ten times as powerful as an X1, and an X1 ten times as powerful as an M1 (the next lowest letter).

“Tachyons are subatomic particles that travel not only at the speed of light, but also all the way up to infinity,” Pars revealed. “The breakthrough came when we detected the Tachyon particles in the northern Aurora Borealis and later also in the southern Aurora Australis. In other words, the solar storms shed plasma containing many charged particles such as electrons and protons that collect in the north and south of the Earth’s magnetic field. These charged particles in the plasma excite the gas in Earth’s atmosphere producing glowing auroras as well as Tachyons in the process. The auroras are in the thermosphere, between five hundred and a thousand kilometers above the Earth.

The Solar Maximum Mission or Solar Max was sent on February 14, 1980. This satellite was accompanied by a lot of scientific instruments, which provided new knowledge and coordinated observations about the nature of solar flares, especially during a period of maximum solar activity. The main purpose of the Solar Max was to investigate the solar phenomena by collecting data which was direct to the storage and release as flare energy, particle acceleration, formation of hot plasma, and mass ejection.

Solar flares, sunspots, and radiation are all things that are on the Sun and are important parts of the weather on the Sun. Solar flares are short outbursts of energy on the sun. Sunspots are dark spots in the sun from the contrast of its surroundings. Radiation from the sun is also known as sunlight. Radiation is a mixture of electromagnetic waves that range from infrared to ultraviolet rays. Solar flares are caused by a sudden release of energy that has been stored in twisted magnetic fields. The energy of a solar flare is equal to ten million volcanic eruptions, and can last anywhere between a couple minutes to hours on end. Solar flares happen in sunspots where the magnetic fields are strong and active. Solar flares release an incredible amount of energy. It takes energy from the sun about eight minutes to reach Earth.

Harmful particles and rays, such as detritus, radiation, and magnetic waves from outer space are constantly bombarding Earth. Solar wind, a rapidly moving stream of electrons and protons from the Sun, is accountable for stripping away ions such as hydrogen and oxygen from a planet’s atmosphere, releasing them into space. The ratio of hydrogen to oxygen being removed from a planet’s surface, due to this phenomenon, is two to one respectively.

The solar wind containing these hot gases races toward the edges of the solar system, and smash in to the magnetosphere. The magnetosphere protects the earth by deflecting most of the solar wind around the planet. Trillions of these charged particles mange to get through and project from the North and South poles. Energy released in this fashion excites atoms of nitrogen and oxygen, which in turn emit pulses of colored light. These formations are called an aurora. The aurora borealis, which are visible in Alaska, are a result of this sort of space storm.

     Have you ever heard of a solar flare? A solar flare exists after a sunspot has existed for a long time and the magnetic lines of force usually become jumbled. As a result of this jumbling, magnetic energy is stored in the Corona (region of atmosphere above the chromosphere). The energy may be released in a spectacular discharge, which is a solar flare. A solar flare can be as wide as 367,000 miles and as high 500,000 miles out into space. A solar flare is nothing more than helium erupting from the sun like a volcano.