claim: Water levels correlate with sunspots.
evidences.evidence_id: Sun:175
evidences.article: Sun
evidences.evidence: Sunspots are visible as dark patches on the Sun's photosphere, and correspond to concentrations of magnetic field where the convective transport of heat is inhibited from the solar interior to the surface.
evidences.votes: NOT_ENOUGH_INFO NOT_ENOUGH_INFO NOT_ENOUGH_INFO
evidences.evidence_id: Sun:183
evidences.article: Sun
evidences.evidence: At this point in the dynamo cycle, buoyant upwelling within the convective zone forces emergence of toroidal magnetic field through the photosphere, giving rise to pairs of sunspots, roughly aligned east–west and having footprints with opposite magnetic polarities.
evidences.votes: NOT_ENOUGH_INFO NOT_ENOUGH_INFO SUPPORTS
evidences.evidence_id: Sun:209
evidences.article: Sun
evidences.evidence: Long-term secular change in sunspot number is thought, by some scientists, to be correlated with long-term change in solar irradiance, which, in turn, might influence Earth's long-term climate.
evidences.votes: NOT_ENOUGH_INFO NOT_ENOUGH_INFO NOT_ENOUGH_INFO
evidences.evidence_id: Sunspot:48
evidences.article: Sunspot
evidences.evidence: Sunspots number is correlated with the intensity of solar radiation over the period since 1979, when satellite measurements became available.
evidences.votes: NOT_ENOUGH_INFO NOT_ENOUGH_INFO NOT_ENOUGH_INFO
evidences.evidence_id: Sunspot:63
evidences.article: Sunspot
evidences.evidence: On longer time scales, such as the solar cycle, other magnetic phenomena (faculae and the chromospheric network) correlate with sunspot occurrence.
evidences.votes: NOT_ENOUGH_INFO NOT_ENOUGH_INFO NOT_ENOUGH_INFO