That is not
the total radiation from the sun, but it is the emission from the sun of what we call coronal ejections which produces the solar wind.
Any variation in
total radiation from the Sun will force an accompanying change in mean - surface temperature.
Not exact matches
The gauntlet Juno ran at Jupiter held many chances for catastrophe: The spacecraft might have been knocked out by intense magnetic fields (at that distance, 20 times stronger than Earth's), ionizing
radiation (a
total dose of 265 rads — more than enough to kill a human being), dust particles
from Jupiter's rings (
from which the main engine was completely unshielded) or loss of power if the solar arrays were unable to reorient to the
sun.
Sunlight can be more technically defined as the
total frequency spectrum of the electromagnetic
radiation emanated
from the
sun.
The temperature around the world is now increasing and TSI (
Total Solar Irradiance) I think solar cycle can cause global warming because our temperature is increasing by
radiation from the
sun which comes
from solar cycle too.
Although only 1 percent of the
sun's energy is emitted at ultraviolet wavelengths between 200 and 300 nanometers, the decrease in this
radiation from 1 July 1981 to 30 June 1985 accounted for 19 percent of the decrease in the
total irradiance over the same period.»
Total solar irradiance - The amount of solar
radiation received outside the Earth's atmosphere on a surface normal to the incident
radiation, and at the Earth's mean distance
from the
Sun.
The recalculation of 0.0163 K / year gives the increase of the power density due to the increase of CO2 in the order of magnitude of 0.1 W / m ^ 2 per year as compared to the
total available average power density of 550 W / m ^ 2 (which includes the mean value of the irradiation
from the
Sun and the back
radiation).
If so, then we can put numbers behind the qualitative discussion on the influence of CO2 on the climate of the Earth since we can now relate the additional heat available due to the absorption of the outgoing
radiation by CO2 to the
total heat available due to the irradiation
from the
Sun and the back
radiation previously to the enriching of the atmosphere by CO2.
Try this for size: http://hyperphysics.phy-astr.gsu.edu/hbase/phyopt/albedo.html Includes this «The bond albedo is the
total radiation reflected
from an object compared to the
total incident
radiation from the
Sun.