The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
The circumstances which accompany the formation of a spot cannot readily
be specified with certainty. It is impossible to say that there exists
any law as to this matter. Whilst some spots develope very slowly by the
expansion of certain pores, others spring into existence quite suddenly.
Yet it cannot be said that the formation of a spot is ever completely
instantaneous however rapid it may be. The phenomenon is often announced
some days in advance: we may perceive in the photosphere a great
agitation which often manifests itself by some very brilliant _faculæ_
(to be described presently) giving birth to one or more pores. Very
often we next notice some groups of little black spots, as if the
luminous stratum was becoming thinner in such a way as to disappear
little by little and leave a large black nucleus uncovered. At the
commencement of the business there is usually no clearly defined
penumbra. This developes itself gradually and acquires a regular
outline, just as the spot itself often takes a somewhat circular form.
This tranquil and peaceable formation of a spot only happens at a time
when calm seems to reign in the solar atmosphere: in general the
development is more tumultuous and the stages more complicated.
As a rule a spot passes through three stages of existence:—(1) the
Period of birth; (2) a Period of calm; and (3) the Period of
dissolution. When a spot is on the point of closing up, the flow of the
luminous matter which it, as it were, attracts, is not directed
uniformly towards the centre; it seems that the photospheric masses, no
longer meeting with resistance, are precipitated promiscuously anywhere
so as to fill up the hole. It is impossible to describe in detail the
phases which irregular spots go through, but two things may always be
remarked: that their structure is characterized by the existence of
luminous filaments, and that these filaments converge towards one or
several centres.
Secchi thus sums up certain conclusions which he arrived at relating to
spots generally:—(1) It is not on the surface of any solid body that the
solar spots are manifested; they are produced in a fluid mass, the
fluidity of which is represented by a gas, so that the constitution of
this medium may be likened to that of flames or clouds; (2) the known
details respecting the constitution of the penumbra and the phenomena
exhibited prove that the penumbra is not a mass of obscure matter which
floats across luminous matter, but that it is on the contrary a case of
luminous matter invading and floating about over darker materials and so
producing a half tint.
Public-domain text, read in full here on John Shaqi.
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