Since yesterday’s bulletin, solar activity was on the C-level, with the strongest flare being the C5.2 flare peaking yesterday at 21:24 UT in the Catania sunspot group 44 (NOAA AR 1255) close to the east-south-east limb. The same active region yesterday produced the M2.5 flare that was accompanied only by a weak and narrow CME. The solar background X-ray flux is currently around the C1 level. We expect flaring activity up the M-level, in particular from the Catania sunspot group 44. The former
NOAA AR 2139 (that was responsible for the major eruption on the far side of the Sun on September 1) is now appearing from behind the east limb. The solar proton flux, although increased, has stabilized below the SEP event threshold. We maintain the warning condition for a proton event. The Earth is currently inside a slow (around 390 km/s) solar wind flow with average (around 5 nT) interplanetary magnetic field magnitude. The geomagnetic conditions are quiet and are expected to remain so.
Equipment: Coronado 90 + Imaging Source DMK + LX75
Processing: Photoshop, Avistack 300 frames
Time UT: 16:00
Exposure 1/500 sec.
Image Credit & Copyright: Rolando Ligustri (CARA Project, CAST)
On October 19th, a good place to watch Comet Siding Spring will be from Mars. Then, this inbound visitor (C/2013 A1) to the inner solar system, discovered in January 2013 by Robert McNaught at Australia’s Siding Spring Observatory, will pass within 132,000 kilometers of the Red Planet. That’s a near miss, equivalent to just over 1/3 the Earth-Moon distance. Great views of the comet for denizens of planet Earth’s southern hemisphere are possible now, though. This telescopic snapshot from August 29 captured the comet’s whitish coma and arcing dust tail sweeping through southern skies. The fabulous field of view includes, the Small Magellanic Cloud and globular star clusters 47 Tucanae (right) and NGC 362 (upper left). Worried about all those spacecraft in Martian orbit? Streaking dust particles from the comet could pose a danger and controllers plan to position Mars orbiters on the opposite side of the planet during the comet’s close flyby.
APOD NASA 04-Sep-14
The Omega Nebula, also known as the Swan Nebula, Checkmark Nebula, Lobster Nebula, and the Horseshoe Nebula (catalogued as Messier 17 or M17 and as NGC 6618) is an H II region in the constellation Sagittarius.
The Omega Nebula is between 5,000 and 6,000 light-years from Earth and it spans some 15 light-years in diameter. The cloud ofinterstellar matter of which this nebula is a part is roughly 40 light-years in diameter and has a mass of 30,000 solar masses. The total mass of the Omega Nebula is an estimated 800 solar masses.
Imaging telescopes or lenses: Officina Stellare Veloce RH200
Imaging cameras: QSI 683WSG
Mounts: Skywatcher N-EQ6 pro
Guiding telescopes or lenses: Officina Stellare Veloce RH200
Guiding cameras: Starlight Xpress Lodestar
Software: PixInsight, Maxim DL
Filters: Astrodon Ha 3nm Tru-Balance, Astrodon OIII
Accessories: Finger Lake Instruments Atlas Focuser
Dates: Aug. 16, 2014, Aug. 17, 2014
Astrodon Ha 3nm Tru-Balance: 14×600″
Astrodon OIII: 6×600″
Integration: 3.3 hours
Author: Davide Manca
AstroPhotography of the day by SPONLI 04 Sep 2014