... Table 6.3: Sky Brightness (V mag arcsec^-2) as a Function of Heliocentric Ecliptic Latitude and Longitude. ... The actual sky brightness depends on the heliocentric ecliptic coordinates (latitude and longitude) in a manner summarized in ...
... V. Note that the sky background is a strong function of position, especially for targets near the ecliptic; the sky level can vary from V=23.3 mag arcsec -2 at the ecliptic pole to about V=20.9 mag arcsec -2 on the ecliptic near the solar avoidance limit ...
... V. Note that the sky background is a strong function of position, especially for targets near the ecliptic; the sky level can vary from V=23.3 mag arcsec-2 at the ecliptic pole to about V=20.9 mag arcsec^-2 on the ecliptic near the solar avoidance limit ...
... V. Note that the sky background is a strong function of position, especially for targets near the ecliptic; the sky level can vary from V=23.3 mag arcsec -2 at the ecliptic pole to about V=20.9 mag arcsec -2 on the ecliptic near the solar avoidance limit ...
... brightness depends on the heliocentric ecliptic coordinates (latitude and longitude ... V mag arcsec-2) as a Function of Heliocentric Ecliptic Latitude and Longitude ... Heliocentric . Ecliptic . Longitude . Ecliptic Latitude . 0њ . ...
... b1rightness depends on the heliocentric ecliptic coordinates (latitude and longitude ... V mag arcsec -2 ) as a Function of Heliocentric Ecliptic Latitude and Longitude ... Heliocentric . Ecliptic . Longitude . Ecliptic Latitude . 0° . ...
... V mag arcsec-2) as a Function of Heliocentric Ecliptic Latitude and Longitude ... positions 45 degrees out of the ecliptic the zodiacal background can be approximated ...