STEVE (Strong Thermal Emission Velocity Enhancement) is an aurora-like phenomenon that can be observed in middle latitudes. STEVE does not belong to traditional auroras as a phenomenon, but may appear at the same time with them.
STEVE looks like a narrow, white or mauve arc that is clearly separate from the rest of the aurora oval in the pole-ward side of the sky. In Northern Europe, STEVE can sometimes be seen quite far from the oval and be visible across the southern half of the sky.
A mauve STEVE with a clear gap to the oval. Image: Keijo Lehtimäki
It forms a long and narrow east-west aligned dim line that goes across the night sky. The length of the arc can be over 2 000 km and it is located at altitudes of 110-300 kilometers.
The best time for observing STEVE is when the active aurora of a substrom have subsided.
The arc is white, grey or light purple in color, but the appearance of the arc may vary slightly. In more colorful versions, the bottom edge of the arc shows while/grey color, whereas the upper part has more purple shade. These colorful versions are called Double-Layer STEVE.
Double-Layer STEVE. Image: Eero Karvinen
STEVE's appearance can resemble single, detached rays or there can be rays within the arc itself.
A ray-like STEVE. Photo by: Riku Talvio
Quite often purple rays within the aurora oval itself get mistakenly identified as STEVE. While within the aurora oval the purple rays tend to disappear relatively fast, STEVE-events can last from ten minutes to hours.
STEVE very rarely shows green color, whereas lower edges oval's traveling rays tend to be clearly green. However, occasionally there may also be a green, "toothed" band called ”picket fence” below and aligned with the STEVE arc.
STEVE with picket fence. Image: Sirpa Pursiainen
SAR arcs are a different phenomenon happening in the same region that sometimes gets mixed up with STEVE. SAR-arcs, however, are more diffuse, dimmer or fainter, purely red, and lasts longer than STEVE, even days.
This rare image shows a red SAR-arc with a white STEVE arc. There is an area without aurora light around STEVE. Image: Atacan Ergin
When photographing a suspected STEVE, it is important to try capturing both the arc form and the arc's location in relation to the rest of the oval.
In some cases, fine westward-moving structures can be observed within the arc. These can be captured by taking videos of the event or capturing short-exposure animations.
Bilderna saknar exif -data när är första bilden med röda bågen tagen? Jag antaar, att den är en SAR -båge i alla fall. När jag har fått klarhet i händelsenrnas ordning, kommen observationen updateras.