Home

About

Advanced Search

Browse by Discipline

Scientific Societies

E-print Alerts

Add E-prints

E-print Network
FAQHELPSITE MAPCONTACT US


  Advanced Search  

 
Astronomy & Astrophysics manuscript no. aa20042579 April 26, 2005 (DOI: will be inserted by hand later)
 

Summary: Astronomy & Astrophysics manuscript no. aa20042579 April 26, 2005
(DOI: will be inserted by hand later)
Time series study of EUV spicules observed by SUMER/SoHO
L. D. Xia 1,2 , M. D. Popescu 2,3 , J. G. Doyle 2 and J. Giannikakis 2,4
1 School of Earth and Space Sciences, Univ. of Science and Technology of China, Hefei, Anhui 230026, China
e­mail: xld@ustc.edu.cn
2 Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
e­mail: [mdp; jgd]@arm.ac.uk
3 Astronomical Institute of the Romanian Academy, RO­75212 Bucharest 28, Romania
4 Sect. of Astrophysics, Astronomy and Mechanics, Dept. of Physics, Univ. of Athens, Athens 15783, Greece
Received / accepted
Abstract. Here we study the dynamic properties of EUV spicules seen at the solar limb. The selected data were
obtained as time series in polar coronal holes by SUMER/SoHO. The short exposure time and the almost fixed
position of the spectrometer's slit allow the analysis of spicule properties such as occurrence, lifetime and Doppler
velocity. Our data reveal that spicules occur repeatedly at the same location with a birth rate of around 0.16/min
as estimated at 10 ## above the limb and a lifetime ranging from 15 down to #3 minutes. We are able to see some
spicules showing a process of ``falling after rising'' indicated by the sudden change of the Doppler velocity sign. A
periodicity of #5 minutes is sometimes discernible in their occurrence. Most spicules have a height between 10 ##
and 20 ## above the limb, and some can stretch up to 40 ## . These ``long macro­spicules'' seem to be comprised of a
group of high spicules. Some of them have an obvious periodicity in the radiance of #5 minutes.

  

Source: Armagh Observatory

 

Collections: Physics