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Skywarden,
Ursa Astronomical Association
Kopernikuksentie 1
00130 Helsinki
taivaanvahti(at)ursa.fi

Ursa Astronomical Association

Half-sky auroras - 20.2.2015 at 23.43 Kemijärvi Observation number 33788

Visibility IV / V


The clouds fell from the sky on Friday during the day, but the forecast for the northern lights was otherwise poor. Well, I decided to try the ice in the evening before the sauna (about 10:30 pm) and there was a very dull gauze there. I took a test shot and was able to confirm the observation. And at about 23 times it started to happen. Belts, gauze, and rays began to appear in the sky in a vague order. Some were very active and some quite passive. The show continued until 0:30 until it started to freeze and the graph froze. The clouds also flew to the scene as early as 0:20.

Then for those who know, the question is: What is wrong with these image settings when another image does not show blue at all?



More similar observations
Additional information
  • Aurora brightness
    • Very bright auroras
  • Colors with unaided eye and other features
    • Streaming auroras info

      Streaming. In streaming aurora fast irregular variations in brightness occur along the horizontal dimension of homogeneous shapes.

    • Flickering auroras info

      Flickering. This rare subclass refers to a situation where irregular variations in brightness occur in aurora, such as in fluttering flames.

    • Flaming auroras info

      Flaming. This rare subclass of aurora does not mean so much a single shape, but a large area in the sky. In the flaming aurora, bright waves that are sweeping upward towards the magnetic zenith emerge in the sky. Very rarely waves can wipe downwards. Bands are usually reported during flaming, less often spots.

    • Pulsating auroras info

      Pulsating aurora. The brightness of the pulsating aurora usually varies rhythmically over a period that can be only a fraction of a second at its fastest, but can also be several minutes. Pulsing usually only occurs in(strong auroral conditions) higher quality shows , especially towards the end of them. However, the pulsation may be followed by yet another eruption. Sometimes the variation in brightness is at the same stage in the whole form, whereby the whole form "turns on and off" at the same time. Pulsation is also found in arches and bands, but above all in spots..

    • Blue auroras info

      Clearly blue auroras can be seen only during the best aurora displays close to the maximum phase or soon after it. Sometimes blue auroras can be seen shortly after the sunset at the top part of the auroral shapes, specially rays. It is created by the mission of the ionized nitrogen molecules created by the suns radiation.

      Strongly colored blue auroras. Photo by Jorma Mäntylä.

      Blue top parts of the aurora. Image by Tom Eklund. 

      Blue top parts of the aurora. Image by Jaakko Hatanpää.

      Partly blue corona. Photo by Tapio Koski.

      Faintly blue top parts of an aurora veil. Photo by Jaakko Hatanpää.

    • Red coloration of the shapes top info

      Auroras which have red top part that can be seen with naked eye are most often observed in the bands and long rays. In this case the lower parts are usually green. If the upper parts are in sunlight, red may be stronger than green. This shade of red is due to the discharge of the excitation state of the atomic oxygen.

      Aurora that shift to reddish towards the top. Photo by Karri Pasanen. 

      Red top in a aurora band. Photo by Simo Aikioniemi.

      Red at the top of the aurora. Picture of Tom Eklund.

    • Green auroras info

      Green, seen with the naked eye, is one the most common colors of the aurora. The green color is derived from atomic oxygen.

      Green auroras. Lea Rahtu-Korpela.

      Green auroras. Photo by Juha Ojanperä.

  • Observed aurora forms
    • ;Veil;Rays;Band;Corona;Arc
Comments: 3 pcs
Janne Kari - 21.2.2015 at 06.51 Report this

Hienoa jälkeä, hyvät kuvat.

Värien vaihtelun suurin syy on varmaankin kameran AWB asetukset, eli kamera on ollut automaattisella valkotasapainon säätömoodilla ja arponut kuvan värilämpötilan sitten jotenkin sinneppäin. Kun värilämpötilaa laskee, niin kuva "sinistyy", nostossa taas väriavaruus lämpenee kohti punaista.

Jos ei kuva raakakuvia vaan JPG:tä, niin värilämpötilaa ei ole jälkikäsittelyssä helppoa säätää enään. Raakakuvissahan sitä voi ihan vapaasti vielä väännellä miten haluaa.

Kannattaa kamerasta tarkistaa WB (white balance) asetukset ja reposkuvauksissa valita "yö" moodi jos kuvaa JPG:tä.

Leo Jussila - 21.2.2015 at 10.14 Report this

No tätä värilämpötilaa epäilin, mutta en millään asetuksilla saanut enää 1. kuvan kaltaisia kuvia. Ja kuvat on onneksi .raw muodossa.

Tommi Lyytikäinen - 21.5.2015 at 17.14 Report this

Heittäisin lonkalta, innokkaana revontulikuvaajana että sensorin valoherkkyys vaikuttaisi tässä tapauksessa asiaan. Itse olen aika aloittelija mitä tulee valkotasapainoon, mutta nuiden kuvien ja omien kokemusten perusteella tuo vastaa täydellisesti ISO asetuksen voimakkuutta. Ykköskuva on otettu korkealla ISO:lla ja kakkonen erittäinkin pienellä. Kannattaa kokeilla ensi kerralla sen asetuksen vaikutuksia. Pitää vielä vertailla omia kuvia.

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