by Kevin Reardon » Tue Nov 02, 2010 11:56 pm
Yes, I've been excusing myself to colleagues all day about the caption. You would be hard pressed to find a clear spicule in the image. This is in large part because the image was taken in Ca II 8542, not H-alpha, and the response of the lines is quite different. This is the corresponding H-alpha image (rotated with respect to the orientation of the APOD image):
You can see the this as well as corresponding photospheric and coronal images (the latter from SDO/AIA) here:
http://www.arcetri.astro.it/science/sol ... S/gallery/
Anyway, the following is the caption we suggested, which waxes poetic as well but contains a bit more useful information:
--------------------
Gateway to the Corona
Explanation: What lies between the solar photosphere, where sunspots can be seen, and the corona, with its magnetic arches stretching outward?
It's the enigmatic solar chromosphere, the region of the solar atmosphere where the magnetic field starts to dominate, forming long, thin, dense structures. The above image shows a large area of the solar chromosphere around active region NOAA 11092 near the center of the Sun on August 3, 2010. This image, taken not in the well-known Hydrogen alpha spectral line, but in a line produced by ionized Calcium in the near infrared, covers a relatively extended area of the solar surface (170,000 km on a side), with a very high spatial resolution (160 km), allowing it show the details of the great diversity of chromospheric structures, including a myriad of fibrils, the sunspot and the small bright flare in the lower left and a filament in the upper right. Away from these fibrils, the small, round brightenings are the signature of sound waves buffeting the chromosphere from below. Complex and dynamic, the chromosphere is the gateway to the corona.
--------------------
kevin reardon
Yes, I've been excusing myself to colleagues all day about the caption. You would be hard pressed to find a clear spicule in the image. This is in large part because the image was taken in Ca II 8542, not H-alpha, and the response of the lines is quite different. This is the corresponding H-alpha image (rotated with respect to the orientation of the APOD image):
[img2]http://www.arcetri.astro.it/science/solare/IBIS/gallery/IBIS/Photos_files/Media/ha6563.mosaic.v3.cln/ha6563.mosaic.v3.cln.jpg[/img2]
You can see the this as well as corresponding photospheric and coronal images (the latter from SDO/AIA) here:
[url]http://www.arcetri.astro.it/science/solare/IBIS/gallery/[/url]
Anyway, the following is the caption we suggested, which waxes poetic as well but contains a bit more useful information:
--------------------
Gateway to the Corona
Explanation: What lies between the solar photosphere, where sunspots can be seen, and the corona, with its magnetic arches stretching outward?
It's the enigmatic solar chromosphere, the region of the solar atmosphere where the magnetic field starts to dominate, forming long, thin, dense structures. The above image shows a large area of the solar chromosphere around active region NOAA 11092 near the center of the Sun on August 3, 2010. This image, taken not in the well-known Hydrogen alpha spectral line, but in a line produced by ionized Calcium in the near infrared, covers a relatively extended area of the solar surface (170,000 km on a side), with a very high spatial resolution (160 km), allowing it show the details of the great diversity of chromospheric structures, including a myriad of fibrils, the sunspot and the small bright flare in the lower left and a filament in the upper right. Away from these fibrils, the small, round brightenings are the signature of sound waves buffeting the chromosphere from below. Complex and dynamic, the chromosphere is the gateway to the corona.
--------------------
kevin reardon