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Twelve days of Helios
19-30 April 2015 in 5 minutes
What's behind
Solar Prominences
and Tornadoes?
Nicolas Labrosse
University of Glasgow
School of Physics & Astronomy
www.astro.gla.ac.uk/?p=171
@niclabrosse
IRIS
Hinode
SDO
SOHO
Crater image by James Stuby based
on NASA Lunar Orbiter 4 image
Edison Pettit 1889-1962
Co-aligning data sets
• Want to examine correlations between parameters on a
pixel-by-pixel basis
• Start by co-aligning data sets:
• AIA
• THEMIS
• IRIS SJI
• IRIS raster
• Hinode SOT
• Hinode EIS
• Co-aligned using 2D cross-
correlation
Co-aligning data sets
Grey = AIA 304 Å
Red = IRIS Mg II SJI
Blue = SOT Ca II
Green = EIS 256 Å
Contour = THEMIS
Thank you spectroscopy!
• Hinode/EIS: spectroscopic look at tornadoes
Spectroscopy
Detailed analysis
of light properties
as a function of
“colour” (ie
wavelength or
frequency)
Thank you spectroscopy!
Nic Labrosse – High-resolution observations of tornado-prominences – EWASS18
Thank you Doppler!
Nic Labrosse – High-resolution observations of tornado-prominences – EWASS18
Thank you Doppler!
Tornado + Prominence Eruption
SDO/AIA
193Å
23-29-Apr-2015
Prominence Eruption
SDO/AIA
304Å + 335Å
31-Aug-2012
19:00 - 24:00
Coronal Mass Ejection (CME)
Expanding magnetic “bubble”
of material breaks off into
space
– Typically a billion tonnes
travelling at million km/h (450
km/s)
If directed towards Earth can
get major geomagnetic storm
– A few days to reach Earth but
tricky to predict
SoHO/Lasco coronograph
ESA’s Solar Orbiter
Multi-wavelength imagers,
spectrometers and in-situ particle
detectors
– University of Glasgow
researchers involved with several
of the instruments
Launches 2020
– Gets closer to the Sun than
Mercury after cruise phase
NASA’s Parker Solar Probe
We live in the Sun’s atmosphere
@niclabrosse
@CafeSciFREcosse

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Solar tornadoes MAD 2018

  • 1. Twelve days of Helios 19-30 April 2015 in 5 minutes
  • 2.
  • 3. What's behind Solar Prominences and Tornadoes? Nicolas Labrosse University of Glasgow School of Physics & Astronomy www.astro.gla.ac.uk/?p=171 @niclabrosse
  • 4.
  • 6. Crater image by James Stuby based on NASA Lunar Orbiter 4 image Edison Pettit 1889-1962
  • 7.
  • 8.
  • 9.
  • 10.
  • 11.
  • 12. Co-aligning data sets • Want to examine correlations between parameters on a pixel-by-pixel basis • Start by co-aligning data sets: • AIA • THEMIS • IRIS SJI • IRIS raster • Hinode SOT • Hinode EIS • Co-aligned using 2D cross- correlation
  • 13. Co-aligning data sets Grey = AIA 304 Å Red = IRIS Mg II SJI Blue = SOT Ca II Green = EIS 256 Å Contour = THEMIS
  • 14. Thank you spectroscopy! • Hinode/EIS: spectroscopic look at tornadoes Spectroscopy Detailed analysis of light properties as a function of “colour” (ie wavelength or frequency)
  • 16. Nic Labrosse – High-resolution observations of tornado-prominences – EWASS18 Thank you Doppler!
  • 17. Nic Labrosse – High-resolution observations of tornado-prominences – EWASS18 Thank you Doppler!
  • 18. Tornado + Prominence Eruption SDO/AIA 193Å 23-29-Apr-2015
  • 19. Prominence Eruption SDO/AIA 304Å + 335Å 31-Aug-2012 19:00 - 24:00
  • 20. Coronal Mass Ejection (CME) Expanding magnetic “bubble” of material breaks off into space – Typically a billion tonnes travelling at million km/h (450 km/s) If directed towards Earth can get major geomagnetic storm – A few days to reach Earth but tricky to predict SoHO/Lasco coronograph
  • 21. ESA’s Solar Orbiter Multi-wavelength imagers, spectrometers and in-situ particle detectors – University of Glasgow researchers involved with several of the instruments Launches 2020 – Gets closer to the Sun than Mercury after cruise phase
  • 23. We live in the Sun’s atmosphere @niclabrosse @CafeSciFREcosse