Spicule (solar physics)
A
spicule is a dynamic jet of about 500km diameter on the
Sun. It moves upwards at about 20 km/s from the
photosphere They were discovered in 1877 by Father
Angelo Secchi of the
Vatican Observatory in Rome,
Spicules live for about 5-10 minutes; at the solar limb they appear elongated (if seen on the disk, they are known as "mottles" or "fibrils"). They are usually associated with regions of high magnetic flux; their mass flux is about 100 times that of the
solar wind.
At any one time there are around 100,000 active spicules on the Sun; an individual spicule typically reaches 3,000-5,000 km altitude above the photosphere.
Bart De Pontieu (
Lockheed Martin Solar and Astrophysics Laboratory,
Palo Alto, California ),
Robert Erdélyi and
James P. Stewart (both from the
University of Sheffield,
Sheffield, UK) showed in 2004 that spicules formed as a result of P mode oscillations in the Sun's surface, sound waves with a period of about five minutes that causes the Sun's surface to rise and fall at several hundred meters per second (see
helioseismology). Magnetic flux tubes that tilted away from the vertical can focus and guide the rising material up into the solar atmosphere to form a spicule.
* De Pontieu, B., Erdélyi, R. and Stewart, J:
Solar chromospheric spicules from the leakage of photospheric oscillations and flows In:
Nature. 430/2004, p. 536â€"539,
