Solar REU 2011 Jewels of the Sun A Statistical Study of X-Ray Bright Point Energetics Tom Elsden...
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Transcript of Solar REU 2011 Jewels of the Sun A Statistical Study of X-Ray Bright Point Energetics Tom Elsden...
Solar REU 2011Jewels of the Sun
A Statistical Study of X-Ray Bright Point Energetics
Tom ElsdenUniversity of St Andrews, Scotland
Talk Outline
• Introduction to X-ray bright points• Purpose of the project• What have we learned?• What’s left to do?
Basic Facts
• What do we know about them?• Lifespan: 2 hours – 2 days• Size : 2-10 x104 km• Found at all latitudes• Temperature :1-2MK• Numbers: 100s – 1000s• Emerging magnetic flux
approximately 10000
Missouri’s!
Purpose of study
• Perhaps small scale tells us of large scale• These little guys are relatively unstudied• Are all XBP’s simple magnetic bipoles?• What energizes them?
Coronal Temperature
•Generally defined > 106 K.
•Sharp rise in temperature, we believe to be caused by strong magnetic fields.
•We can see the wavelengths used to observe bright points.
Image, Astronomy and Astrophysics
In the beginning…
• Analysed the magnetic field in the photosphere.
• Observed that this was not going to be as simple as first planned.
• ‘Simple bipoles’ didn’t quite cover it.
Aims• Bright point temperatures
• Surrounding environment effects.
• Orientation
• Tangential flow in photosphere surrounding magnetic islands*
• Magnetic flux vs emission
We see a relatively normal distribution, with a gap to higher temperature BP’s caused byusing the 211 filter for higher temperature bright points rather than 171 or 193.
OrientationJoy’s Law & Hale’s law
Expect two peaks at 315-360 & 180-225 degrees in top plot.
Expect one peak at 315-360 degrees in bottom plot.
Future Work
• Do more statistics!• Much more can be done with the flow maps,
magnetic flux and temperature correlations.• Apply to much more data.