SOLAR FILAMENT

SOLAR2jpg-91804e9

FERNANDO OLIVEIRA DE MENEZES

SAO PAULO

Equipments:
Apo 150mm triplet
Asi 174mm
Daystar Cromosphere + ERF
Date: June 24, 2018
Sao Paulo-SP

SOLAR FILAMENT

They are regions colder than the neighborhood plasma and are held in place by the force of the intense magnetic field.

Because they are cooler than the neighboring regions, the filaments appear in h-alpha images as darker traces. For ease of observation, the recorded scene displays the inverted colors, highlighting the fainter details.

2018-06-24T00:00:00

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