Showing posts with label Sun. Show all posts
Showing posts with label Sun. Show all posts

Wednesday, March 11, 2026

Solar Observation Indices: White Light vs. H-alpha

 

I was inspired by the VVS Solar Working group organised last Sunday, March 8, 2026 on the determination of H-Alpha activity on the Sun using indices. Going through some of my books like "Die Sonne beobachten" from Beck and Völker (see aswell link to my books) and a couple of websites I made following list on potential use of H-alpha indices. I made a reference towards white light observation.




Sunday, March 1, 2026

Corona


The corona is the outermost layer of the solar atmosphere, consisting of extremely tenuous and very hot plasma.

- Plasma: H⁺ and e⁻
- Follows magnetic structures
- Temperature anomaly:
        - Magnetic reconnection provides the basic heating
        - Alfvén waves (wave heating) transport energy further out into space
- Radiation spectrum: X-rays (RX), EUV, and white light due to electron scattering
- Density: ~10⁻¹² of the photosphere
- Charged particles escape from the corona and move through our solar system as the solar wind.




We can destiguish different regions:


E Corona (L Corona – Line Corona)
Emission from highly ionized metals (Fe XIV, Ni XII, Ni XIII, Ca XV).
Ionization occurs at t = 2 million K.



K Corona
Thomson scattering by high-energy electrons.
The scattering does not affect the wavelength itself, but the electrons’ velocities cause a Doppler effect, which smears out the wavelengths and thus forms a continuous spectrum (continuum).

F Corona
Caused by dust that scatters photospheric light.
No change to the spectrum shape, and it shows an absorption spectrum; hence the Fraunhofer-line spectrum.




Thursday, February 19, 2026

Differential Velocity of the Sun - JSolex 4.5 release

With the release of JSolex 4.5, it's now possible to calculate the differential velocity of the sun's disk using doppler effect of H-alpha.
I used some of my better Sol'Ex images and the result is very good compared with the theoretical one.






Sunday, January 18, 2026

PRO-AM Collaboration for Systematic Solar Observations

 

PRO-AM Group | JASON2025


Systematic observations of the solar chromosphere and photosphere began 117 years ago at the Meudon Observatory with the spectroheliograph developed by Deslandres. Since then, an exceptional collection of more than 90,000 monochromatic images in Ca II K and Hα has been built up, covering over 11 solar cycles. This unique dataset is made available to the international scientific community through the BASS2000 database.

In 2023, this long observational tradition received new momentum with the launch of a “PRO-AM” collaboration between professional and amateur astronomers. This initiative makes use of the Solar Explorer (Sol’Ex), a compact, high-quality spectroheliograph designed by Christian Buil. The aim of the collaboration is to record solar images on a daily basis, and whenever possible several times per day. Thanks to dozens of observing stations distributed across different geographical locations, the impact of local weather conditions is significantly reduced.

Meanwhile, the range of available spectroheliographs has been further expanded. In addition to the original Sol’Ex, Sol’Ex Pro, Sol’Ex V2, Sol’Ex by James R, Sol’Ex original, and the SHG700 are now available, enabling amateurs with diverse technical backgrounds and resources to participate in the project.

In 2025, a total of 59 amateur astronomers were actively involved in the PRO-AM collaboration. The majority of them, 39 participants, were based in France, while the others were spread across nine additional countries. Together, they were responsible for no fewer than 4,548 observations in various spectral lines, including Hα, Hα 2cb, Ca II H (H3), Ca H1v, Ca II K (K3), and Ca K1v.

Thanks to the strong commitment of the amateur community, there was only a single day in 2025 without an Hα observation, namely 22 December. For Ca II H and Ca II K observations, however, the number of days without data remains significantly higher, highlighting the importance of further expanding the observing network.

Within this international collaboration, I am currently still the only Belgian amateur actively submitting images to the Meudon Observatory. In total, I submitted 82 observations in 2025, placing me seventh among the most active amateur contributors. For the specific Ca II H and Ca II K lines, I rank fourth and fifth respectively. This clearly demonstrates not only the value of individual dedication, but also the crucial role amateur astronomers play in achieving long-term, continuous solar monitoring.

Saturday, January 10, 2026

Sun May 2025 Sphere Synoptic - Inti Partner and Naming _YYYY-MM-DDTHH-MM-SS

I installed the new verion 1.2 of Inti Partner which has a tab Synoptic. It's possible to create a mp4 or GIF file made from solex images over multiple days. The end result is a simulation of the sun's rotation. I had some issues with the error "Date Error" but this is now fixed:

1) only use PNG/fits/ files
2) make sure the Log file is available at the same or upper map
or 
1) if you don't have the Log file, change the naming of the file to following format:
_YYYY-MM-DDTHH-MM-SS_  
2) be aware to change timing to UT time

I used files from May 2025: May 30, 19, 14, 11 and May 2nd. The synoptic maps identified 21 active regions from AR 4070 till AR4103

AR 4070 lat=-12.0° lonCarr=10.0°
AR 4072 lat=-19.0° lonCarr=325.0°
AR 4076 lat=5.0° lonCarr=305.0°
AR 4079 lat=8.0° lonCarr=244.0°
AR 4081 lat=7.0° lonCarr=213.0°
AR 4082 lat=-9.0° lonCarr=188.0°
AR 4084 lat=-21.0° lonCarr=129.0°
AR 4085 lat=3.0° lonCarr=139.0°
AR 4086 lat=7.0° lonCarr=207.0°
AR 4087 lat=15.0° lonCarr=57.0°
AR 4089 lat=17.0° lonCarr=28.0°
AR 4090 lat=-13.0° lonCarr=20.0°
AR 4091 lat=-13.0° lonCarr=33.0°
AR 4092 lat=-13.0° lonCarr=337.0°
AR 4094 lat=20.0° lonCarr=332.0°
AR 4096 lat=6.0° lonCarr=306.0°
AR 4099 lat=-13.0° lonCarr=255.0°
AR 4100 lat=8.0° lonCarr=243.0°
AR 4101 lat=3.0° lonCarr=259.0°
AR 4102 lat=-22.0° lonCarr=297.0°
AR 4103 lat=-17.0° lonCarr=287.0°




Sunday, January 4, 2026

Sun January 4th

A 5cm layer of snow and a perfect blue sky. Sol'Ex time :)
My SSM3 Seeing monitor registrated very good seeing with levels below 1 arcs with sometimes below 0,5arcs. I still have issues with my allignment of the spectral lines which are curved. Maybe I need to adjust the slit? 

Setting: TLAPO80/480 with Sol'Ex by James R and ASI678MM
2nd Gen slit and Herschel Wedge
Tilt <0,5° and Sx/Sy 1,15
SSM3 seeing Monitor via SharpCap
Software: SharpCap, Inti, JSol'Ex, CS4, DeNoise AI










Friday, January 2, 2026

Sun January 2nd

My first observation of the Sun this year.
Moderate conditions and settings of Sol'Ex not perfect, mainly the north side of the Sun.

Setting
Sol'Ex by James R, TLAPO80/480 with ASI678MM
Tilt < 0,1° Sx/Sy 1,04
2nd Gen slit and Herschel Wedge
Software: SharpCap, Inti, JSolex 4.4.2 and CS4






Monday, December 29, 2025

Sun on December 28

The Sun on December 28, 2025. Interesting is the Magnesium Mg I B2 line with a small prominence.

Setting: Sol'Ex by James R, with 2nd Gen slit and Herschel Wedge
Software: SharpCap, Inti, JSol'Ex, CS4, DeNoise AI
Tilt < 0,2° Sx/Sy 1,1









 

Friday, December 19, 2025

Sol'Ex JSolEx 4.4 3D

JSolex version 4.4 creates a 3D image of the Sun using an image made with Sol'Ex.


SOLAP Sol'Ex

Nice feedback from SOLAP project: 

I wanted to thank you because this is the first year since the SOLAP
collaboration that we will have at least one shot per day in Ha in
BASS2000. We're not quite at 100% for CaH and CaK, but it's much better too.

Even even if we didn't have that feeling, 2025 was a good year in terms
of sunshine in Meudon. You have to go back to 2011 to find a better year.

I am taking a few days off, but you can still submit your photos during
this period. I will process them when I return on 31 December.

I wish you all a very happy holiday season.

Florence


Wednesday, December 17, 2025

Adjusting GEN2 slit Sol'Ex

Summary of  NOTICE projet Sol’Ex Le réglage fin du système collimateur Christian Buil

Adjusting a spectroheliograph is less straightforward than it may seem at first, because the camera focus and the light collimation influence each other. A spectrum can look sharp while astigmatism is still present — a tricky optical error where the image is sharp in one direction but not in the perpendicular one. For that reason, a step-by-step, iterative adjustment is required, alternately refining the camera focus and the collimator setting.

To make astigmatism clearly visible, a simple yet clever solution is used: an artificial field edge. By covering roughly half of the slit with a very thin piece of aluminium foil, a sharp transition is created. This makes it possible to judge the sharpness of both the spectral lines and the edge at the same time. Repeating this process a few times leads to an optimal and permanent adjustment — and that directly translates into better solar images.

With the GEN2 slit, an additional challenge appears. At 6 mm, this slit is relatively long, while the Sol’Ex optics were originally designed for a shorter slit. Toward the ends of the GEN2 slit, other optical aberrations become significant and can make focusing misleading. This is exactly where the aluminium-foil method proves its value: by using only the central, optically most reliable part of the slit, these disturbing effects are greatly reduced, allowing accurate collimation.

With the GEN1 slit, the slit itself is shorter and edge-related issues are less pronounced, but there is a different limitation: the chrome-coated surface of the slit is not accessible. As a result, the aluminium-foil mask cannot be applied, and this practical method for reliably checking and correcting astigmatism cannot be used.









Sunday, December 7, 2025

Sol'Ex update with 61 sessions and 962 video shoots

 


My Sol'Ex journey started back in August '23 and today I'm looking back ... a steep learning curve, 3 Sol'Ex versions, 2nd Gen Slit, new 678MM camera, improved software, two conferences, a VVS Whatsapp group, contributing to ProAm Paris Meudon (Bass2000), 2 articles in VVS magazine Heelal, 8 lectures but most impressive my 61 Sol'Ex sessions with 962 video shoots. 

Friday, December 5, 2025

Sun AR4294 4296 4298

Clouds dissapeared for a short time, allowing me to photograph the Sun. Why? Beacuse of a couple of huge sunspots: AR4294, 4296 and 4298. Size are 1280MH, 650MH and 100MH. 

Setting:
TAL200K f/8.5, ASI290MM and Nikon D7500
ND3.8, OIII filter and IR/UV cut filter
Software: SharpCap, AstroSurface, CS4





Friday, November 14, 2025

Sun with Sol'Ex November 8th

A clear sky and enough time for adjusting sharpness. Solution was found in getting the spectrum line in the middle of the space; I get sharpest images when both edges are sharp. Once this was done, I make sure the dustlines on the grating are well seen. 

Setting: TLAPO80/480 with Sol'Ex by James R. and ASI678MM
2nd Gen Slit and Herschel Wedge
Software: SharpCap, Inti V7.0.3, CS4, DeNoise AI
Tilt 0,09°; Sx/Sy 1,09
SSM3 with avg < 1,5arcs whole morning






Sunday, October 26, 2025

Sun October 26

A small opening in the clouds and windy, but still I took my chance resulting in only one capture of the Sun. Some nice prominences at the east side.

Setting: Sol'Ex by James R, 2nd Gen Slit, ASI678MM, TLAPO80/480
Herschel Wedge
Tilt: -0,7° Sx/Sy 1,12
Software: SharpCap, JSolex, Inti, CS4




Sunday, October 12, 2025

Sol'Ex articles published in Magazine Heelal

My articles on Sol'Ex (a follow up article on the evolution of Sol'Ex and it's software)  and the observation of the E-Corona using my Sol'Ex are published in magazine Heelal.


Sunday, September 28, 2025

Sun H-Alpha with active prominences September 29, 2025

 

On the North Eastern limb a free prominence and on the Mid Western limb a long prominence moving away to space... so very active prominences.
The image was processed using new JSolex 4.1.1


This CaIIH is a very sharp image taken with Solex by James R. and 2nd Gen Slit. 
Getting this sharp image is done with both:
- sharp edges
- camera sharpness
- collimator adjustment with focus on the dustlines; this seems working. 



H-alfa2cb



Setting:
TLAPO80/480 with ASI678MM and Solex by James R.
Herstel Wedge
Software: SharpCap 4, Inti 6, JSolex 4.1.1 and CS4
Tilt <0,2° and Sx/Sy 1,1
Seeing with SSM3 almost all day <1,5 arcs
Data submitted to ftp.obspm.fr SOLAP




Saturday, August 30, 2025

Sunspot AR4197

Sunspot AR4197 consists of about 50 spots and is 740MH big. Late afternoon clouds started to disappear and I installed my TAL200K. My parents were at home and I let them watch the big sunspot. Next I connected my ASI290MM camera and took some images. Seeing wasn't good which resulted in more then 500Gb of data. Stacking was done using AstroSurface but editing was done with IMPPG and CS4.

Setting: TAL200 f/8.5, barlow x2 and ASI290MM
Filters : ND5.0, IR/UV cut and OIII
Software: SharpCap, AstroSurface, IMPPG and CS4





 

Sunday, August 24, 2025

Sun August 24, 2025

The Sun this morning (August 24, 2025). Some more 
adjusting of my new Sol'Ex by James R. 
Seeing was < 1,5arcs but at noon time this was increase to 2,5arcs.

Setting: TLAPO80/480 with ASI678MM and Sol'Ex by James R with 2nd Gen slit
Herschel Wedge
Tilt < 0,25° and Sx/Sy 1,1
Software: SharpCap, Inti, JSolex and CS4
Seeing SSM3 on SharpCap