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Over the lifetime of the Sun, the surface rotation rate has decreased significantly. This loss of rotation is thought to have been caused by interaction of the Sun's surface layers with the escaping solar wind. The wind is considered responsible for the tails of comets, along with the Sun's radiation.The solar wind contributes to fluctuations in celestial radio waves observed on the Earth, through an effect called interplanetary scintillation.
From May 10 to May 12, 1999, NASA's Advanced Composition Explorer (ACE) and WIND spacecraft observed a 98% decrease of solar wind density. This allowed energetic electrons from the Sun to flow to Earth in narrow beams known as "strahl", which caused a highly unusual "polar rain" event, in which a visible aurora appeared over the North Pole. In addition, Earth's magnetosphere increased to between 5 and 6 times its normal size.
Both the fast and slow solar wind can be interrupted by large, fast-moving bursts of plasma called interplanetary coronal mass ejections, or ICMEs. ICMEs are the interplanetary manifestation of solar coronal mass ejections, which are caused by release of magnetic energy at the Sun. CMEs are often called "solar storms" or "space storms" in the popular media. They are sometimes, but not always, associated with solar flares, which are another manifestation of magnetic energy release at the Sun. ICMEs cause shock waves in the thin plasma of the heliosphere, launching electromagnetic waves and accelerating particles (mostly protons and electrons) to form showers of ionizing radiation that precede the CME. When a CME impacts the Earth's magnetosphere, it temporarily deforms the Earth's magnetic field, changing the direction of compass needles and inducing large electrical ground currents in Earth itself; this is called a geomagnetic storm and it is a global phenomenon. CME impacts can induce magnetic reconnection in Earth's magnetotail (the midnight side of the magnetosphere); this launches protons and electrons downward toward Earth's atmosphere, where they form the aurora.
"It is vitally important to realize that the 'quiet' sun really isn't all that quiet," says Rich Behnke, program director in NSF's Division of Atmospheric Sciences. "These high-speed streams of wind can affect many of our communications and navigation systems. And they can come at any time, during any part of the solar cycle." When those streams blow by Earth, they intensify the energy of the planet's outer radiation belt. This can create serious hazards for Earth-orbiting satellites and affect global communications systems, while also threatening astronauts in the International Space Station.
Auroral storms light up the night sky repeatedly at high latitudes as the streams move past, driving mega-ampere electrical currents a few hundred miles above Earth's surface. All that energy heats and expands the upper atmosphere. This expansion pushes denser air higher, slowing down satellites and causing them to drop to lower altitudes. The authors note that more research is needed to understand the impacts of these high-speed streams on the planet. The study raises questions about how the streams might have affected Earth in the past when the sun went through extended periods of low sunspot activity, such as a period known as the Maunder minimum that lasted from about 1645 to 1715.
Yes, the solar wind will exert a pressure on objects in interplanetary space, but I believe the pressure of sunlight, small as it is, is greater. It is very rarefied--about 6 atoms per cubic centimeter at the Earth's orbit.
The solar wind does move ion tails in comets, not by colliding with them but by the magnetic field lines embedded in it--a collective effect, in which a large volume of the solar wind acts together.
The solar storm of 1859, also known as the 1859 Solar Superstorm,[1] or the Carrington Event,[2] was a powerful geomagnetic solar storm in 1859 during solar cycle 10. A solar flare and/or coronal mass ejection produced a solar storm which hit earth's magnetosphere and induced the largest known geomagnetic solar storm, which was observed and recorded by Richard C. Carrington.
From August 28, 1859, until September 2, numerous sunspots and solar flares were observed on the sun. Just before noon on September 1, the British astronomer Richard Carrington observed the largest flare,[3] which caused a major coronal mass ejection (CME) to travel directly toward Earth, taking 17.6 hours. Such a journey normally takes three to four days. This second CME moved so quickly because the first one had cleared the way of the ambient solar wind plasma.[3]
Originally posted by piequal3because14
Yes, the solar wind will exert a pressure on objects in interplanetary space, but I believe the pressure of sunlight, small as it is, is greater. It is very rarefied--about 6 atoms per cubic centimeter at the Earth's orbit.
That rock is made of an uncertain material and it has own kinetic energy.
So a rock many millions of times heavier than a satellite will also not be affected.
Sorry no scaremongering.
Anyway, do we have to go through all this exact same scaremongering every time there is a rock near earth?
Something like that and more.
Are you saying that if the Solar Wind(s) are weaker than normal then that will allow the comet to intercept a path toward Earth that isn't calculated for?
We shall see by event.
Originally posted by lostbook
reply to post by piequal3because14
What do you mean?
Correct, they're not to a problematic degree.
Originally posted by alfa1
Recall also that if the solar wind (and CME's) could move objects to any problematic degree, then ALL spacecraft out there would also be affected.
Satellites in geo. orbit, lunar and inner orbit planetary craft, etc...
But they're not.