2014年4月4日-4月6日 太陽光球面 黒点觀測和定位
Solar spherical and sunspots observation test pattern from April 4 to 6, 2014
1. Transfer the digital monocular solar image to the computer (the east-west line of the sun has been corrected as the standard)/the observation instrument is 8 cm Nikon f1200mm+HM25mm eyepiece projection
2. Process the solar image into a standard grayscale photosphere, east-west line, and use the image as a pixel (1000x800PIXELS) for software processing
3. The image is transmitted to the sun positioning software for processing.
4. After the longitude and latitude lines are input into the image, image processing and basic data such as positioning and observation time are performed.
5. Record the overall image.
6. Sunspot recording paper processing
NIKON 8cm refractor + GOTO HM 25mm eyepiece (48x) projection magnification photography
*. The atmospheric disturbance taken from the 4th to the 6th was extremely poor, especially on the 6th.
*.Solar longitude and latitude calculation 5-day data pattern
*.太陽経度緯度計算5日データパターン
PHOTOSHOP 処理された画像と太陽緯度経度測位ソフトウェア
PHOTOSHOP processed images and solar latitude and longitude positioning software (as shown below)圖1