A Photo Of Saturn. Took By Cassini With COISS On February 13, 2007 At 06:45:16. Detail Page On OPUS Database.

A Photo Of Saturn. Took By Cassini With COISS On February 13, 2007 At 06:45:16. Detail Page On OPUS Database.

A photo of Saturn. Took by Cassini with COISS on February 13, 2007 at 06:45:16. Detail page on OPUS database.

More Posts from Read-a-me-to-me and Others

7 years ago

and speak to me from the depths of this long night as if we were anchored here together, tell me everything, chain by chain, link by link and step by step,

Pablo Neruda, from section “XII,”  of excerpts from Heights of Macchu Picchu, transl.Tomás Q. Morín, Plume (August 2017)


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7 years ago
“The Erosive Work Of Streams.”  Elementary Physiography. 1910. 

“The erosive work of streams.”  Elementary physiography. 1910. 


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7 years ago
“Tongues Of Flame Up To A Mile High Leap Out From The Surface Of The Sun.” Children’s Science Book.

“Tongues of flame up to a mile high leap out from the surface of the Sun.” Children’s science book. 1947


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7 years ago
Https://instagram.com/p/BHMsajfj9M7/

https://instagram.com/p/BHMsajfj9M7/


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7 years ago
The Very Last Image From Cassini, Showing Saturn’s Atmosphere & Rings As The Probe Closed In On The

The very last image from Cassini, showing Saturn’s atmosphere & rings as the probe closed in on the planet. *snif*


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7 years ago
Aragonite With Barite - Brixlegg - Schwaz, Inntal, Tyrol, Austria
Aragonite With Barite - Brixlegg - Schwaz, Inntal, Tyrol, Austria

Aragonite with Barite - Brixlegg - Schwaz, Inntal, Tyrol, Austria


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7 years ago
Coronal Prominence Cavity

Coronal Prominence Cavity

  Prominences are regions of cool, condensed plasma supported by twisted magnetic field lines that globally wrap around an axial magnetic field, called a  magnetic flux rope. Most of the flux rope volume is filled with depleted coronal plasma and forms a transitory cavity – a dark elliptical or semi-circular region that appears empty from our viewpoint. White-light coronagraph observations suggest that cavity density is approximately half the density of the surrounding streamers. However, the plasma properties within the cavities are not uniform, they exhibit temperature substructures that have been observed in multiple wavelengths.

Tuned to observe emission in the extreme ultraviolet (EUV or XUV), NASA’s Atmospheric Imaging Assembly (AIA) instrument on board the Solar Dynamics Observatory (SDO) provides high-definition imagery of the Sun in seven wavelength passbands. Each of the wavelengths highlight a specific aspect of the solar surface and atmosphere, for example; the dark elliptical structure of the coronal cavity, and outer bright streamers are most visible in AIA 211 Å (Fe XIV), and AIA 193 Å (Fe XII, XXIV) channels, as shown below:

image
image

The AIA 171 Å (Fe IX) channel also shows the fine structure of loops, plus the central prominence:

image

In the 304 Å (He II) channel only the chromospheric features are visible:

image

More information:

Thermal Properties of a Coronal Cavity (PDF)

SDO/AIA Detection of Solar Prominence Formation Within a Coronal Cavity 

Modeling Coronal Cavities

Image Credit: NASA/SDO/LMSAL


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7 years ago
Eartha Kitt

Eartha Kitt

Istanbul, c. 1949


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7 years ago
Midnight Sun At Lake Luossajärvi. Kiruna, Lappland, Sweden. Original Postcard, Tinted. 1940-1959. Swedish

Midnight sun at Lake Luossajärvi. Kiruna, Lappland, Sweden. Original postcard, tinted. 1940-1959. Swedish National Heritage Board.


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