[HCARC] Tech Corner for May - references
Kerry Sandstrom
kerryk5ks at hughes.net
Sat May 9 22:03:27 EDT 2015
Hi Guys,
Here are the web sites I use:
www.SolarMonitor.org
www.lmsal.com/solarsoft/last_events
www2.hao.ucar.edu/mlso/mlso-home-page
sidc.oma.be
umbra.nascom.nasa.gov/newsite/images.html
www.txarmymars.org/resources/solarweather.php
I usually start with the TX Army MARS site as it includes most of the
data I use from several sites. The SIDC site has sunspot drawings and
often a short article on some aspect of solar activity. It is located
in Belgium. The NASA site is where I get the 171 and 304 Angstrom
images as well as the magnetic field image and the visible image. The
images on this site are all from a satellite. Most of these spectral
lines can't get through our atmosphere. The MLSO site is Muana Loa in
HI. That is where I get the H-alpha images. I usually go to the GONG
H-alpha area and that lets me see the latest images from whichever sites
are currently seeing the sun. There are sites from Australia, HI,
Spain, Chile, CA, etc. Almost always someone has a clear view of the
sun. One choice is to see a "movie" of a period of time when events
occurred. The Solar Soft site is Lockheed-Martin. The main thing I get
hear is a list of recent flares although there is a lot of other
interesting data here. The Solar Monitor site has a lot of images and
other data that is from other sites. It is a different presentation of
the data.
A couple cautions - the sunspot plots are reversed relative to the
images. I guess it is historical. The sunspot plot guys try to make
their data compatible with the sunspot observations of a hundred or more
years ago. They use small telescopes and don't use the magnetic field
data to classify the groups. I don't use the sunspot plots much
myself. Better data is available. You will see lots of mentions of
CME's (Coronal Mass Ejections). Most of what gets ejected is protons.
The solar wind is primarily protons and is hitting us all the time.
There are about a thousand CME's a year on average. During periods of
high solar activity there are more and during low periods there are
less. Only a very small percentage actually hit the earth and of those
most have very minor effects. a CME is nothing to really be concerned
about.
If you have any questions, send me an e-mail. I enjoyed talking to you
all about the sun and propagation and perhaps we can have a follow on
session if you would like.
Kerry
More information about the HCARC
mailing list