Custom Search
Home.
Weather & Health.
Indoor Air Quality.
Noise Pollution.
Urban Heat.
Space Weather.
Cloud Atlas.
Cloud Gallery.
FAQ.
© Global Bioweather 2007  mail@globalbioweather.com

About Us     Contact Us     Disclaimer

Space weather

Forecast

Sunspots

Solar activity

Solar flares

Coronal mass ejection

Solar wind

Magnetosphere

Plasma clouds

Ionosphere

Auroras

Aurora mythology

Mood and depression

Strokes

Migraine

Heart attacks

K-Index

Sitemap

Heat rash

Heat exhaustion

Heat cramps

Rhabdomyolisis

Dehydration

Heatstroke

 

Cold and health

Cold diuresis

Cardiovascular disorders

Common cold and influenza

Raynaud’s disease

Frostnip

Frostbite

Trench foot

Hypothermia

Sun and health

Sunburn

Photoaging

Photosensitivity

Moles, venous lakes

Skin cancer

Macular degeneration

Solar maculopathy

Keratopathy

Cataracts

Eye cancer

Seasonal Affective Disorder

 

Indoor air quality

Outdoor Pollutants

Human Activity

Building material and furniture

Quick reference chart

Tobacco smoke

Bacteria

Dust mites

Cockroaches

Animal dander

Molds

Humidifier fever

Legionnaires’ disease

Sick building syndrome

Multiple chemical sensitivity

Allergies

Radon

Asbestos

Combustion products

Carbon monoxide

Sulfur and Nitrogen dioxide

Particulate matter

Wood heaters

Chemical pollutants

Formaldehyde

Pesticides

Solvents

Fragrances

 

Noise Pollution

How do we hear

Hearing mechanics

The human ear

Pinna

Middle ear

Inner ear

Noise annoyance

Emotional factors

Physical factors

Immune system

Melatonin

Healing process

Cardiovascular disease

The unborn child

Hearing loss

Tinnitus

What is too loud?

Hearing loss prevention

Urban heat island effect

Heat island

How and when

Heatwaves

Heat mortality

Winter benefits

Measuring heat islands

Risk groups

Cool roofs

Building recommendations

The albedo effect

Heat absorption

Passive cooling

FORECASTS: Australia, Belgium, Canada, Denmark, Estonia, Finland, Ireland, Lithuania, Luxembourg, Latvia, Netherlands, Norway, New Zealand, Kaliningrad, Sweden, United Kingdom, United States

Homepage

 

Weather and health

 

Weather sensitivity

Asthma

Hay fever

Headaches & migraine

Rheumatism

Infectious diseases

 

Heat and health

Skill Impairment

Conception and birth

Food poisoning

Low blood pressure

Swollen legs

 

Cloud Atlas

Low clouds

Midlevel clouds

High clouds

 

Cloud gallery

 

 

FAQ

 

Links

Manfred Kaiser

Basicdomestics

My-Zodiac

My Cross Stitch

My Australia

Sitemap
Download How the weather affects your health

Download

The Magnetosphere

The Magnetosphere

In reality, the action of the solar wind changes this picture rather dramatically. The axis of the field is tilted by about 11 degrees to the axis of rotation of the Earth. No one knows why, but these kinds of tilts are found among the magnetic fields of some of the other planets, too.

 

On the daytime side, the field is pushed in by the solar wind pressure, and on the nighttime side, it is invisibly stretched out like a comet's tail. Scientists call the region near the Earth where its field controls the motions of electrically charged particles the magnetosphere. As the Earth rotates, and as the solar wind and coronal mass ejections buffet it from the outside, the magnetosphere trembles and can become stormy. When these rapid, though subtle, changes happen, compass bearings can become unreliable by up to several degrees at the Earth's surface. In space, even more dramatic changes can happen.

 

When the solar wind and the magnetosphere are taken together as a system, they operate like a set of powerful, but invisible, valves that open and close depending on their polarity. When the solar wind's magnetic field is of the south-type polarity, it meets up with the south-type polarity of the Earth's magnetic field. On the daytime side of the Earth, these fields reconnect, causing a transfer of particles and magnetic energy into the Earth's magnetosphere from the solar wind. Severe 'magnetic storms' are triggered, and these can be easily seen even at ground level with sensitive magnetic field detectors called magnetometers.

Changes in the solar wind and in the magnetosphere can also cause the magnetotail region to change in complex ways. The magnetotail resembles a comet's tail and is stretched by the solar wind into a vast cylinder of magnetism nearly one million kilometers long. Magnetic fields in the magnetotail can snap like rubber bands and reconnect themselves, but this time the particles flow down these field lines and plunge deep into the interior of the magnetosphere cavity.

 

Some of these particles can take up temporary residence in an equatorial zone called the ring current. In this vast, invisible river nearly 40,000 kilometers wide, positively-charged particles flow westwards and negatively-charged particles flow eastwards like two trains on opposite tracks. In fact, the flows are so dilute that they actually occupy the same space. Other particles from the magnetotail ride the field lines deep into the Earth's atmosphere and create beautiful aurora.

Source:NASA

Previous

Next

Index

Every square foot of the Earth is pierced by a line of magnetic force, which loops from deep inside the Earth, and far into space, only to return back in a great closed circuit thousands of miles away. If there were no Sun or solar wind, the Earth's magnetic field would extend far beyond the orbit of the moon and millions of kilometers into interplanetary space, in the same shape as a bar magnet field outlined by iron filings.