Still in "Plan of the Investigation", now the second paragraph.
From Euclid to Legendre (to name the most famous of modern reforming geometers) this darkness was cleared up neither by mathematicians nor by such philosophers as concerned themselves with it. The reason of this is doubtless that the general notion of multiply extended magnitudes (in which space-magnitudes are included) remained entirely unworked. I have in the first place, therefore, set myself the task of constructing the notion of a multiply extended magnitude out of general notions of magnitude. It will follow from this that a multiply extended magnitude is capable of different measure-relations, and consequently that space is only a particular case of a triply extended magnitude. But hence flows as a necessary consequence that the propositions of geometry cannot be derived from general notions of magnitude, but that the properties which distinguish space from other conceivable triply extended magnitudes are only to be deduced from experience. Thus arises the problem, to discover the simplest matters of fact from which the measure-relations of space may be determined; a problem which from the nature of the case is not completely determinate, since there may be several systems of matters of fact which suffice to determine the measure-relations of space - the most important system for our present purpose being that which Euclid has laid down as a foundation. These matters of fact are - like all matters of fact - not necessary, but only of empirical certainty; they are hypotheses. We may therefore investigate their probability, which within the limits of observation is of course very great, and inquire about the justice of their extension beyond the limits of observation, on the side both of the infinitely great and of the infinitely small.
Hoo boy.
From Euclid to Legendre (to name the most famous of modern reforming geometers) this darkness was cleared up neither by mathematicians nor by such philosophers as concerned themselves with it.
So Riemann's saying that the mathematical accounts in history, while possibly providing different conceptions of space (as comparing Euclid to Legendre and later Gauss), did little to remove the void of darkness between mathematical intuitions of space and their axiomatisations; to name the darkness, I think it is characterised by the questions: "What do our intuitions (1) say about the axioms (2)? And what do the (2) axioms say about our intuitions (1)?", characterising the relationship between (1) and (2) from both sides as it were.
The reason of this is doubtless that the general notion of multiply extended magnitudes (in which space-magnitudes are included) remained entirely unworked.
Space magnitudes seem to be treated as 0 dimensional points, 1 dimensional lines, 2 dimensional areas and 3 dimensional volumes. Space-time in the Einsteinian sense would also be a 'multiply expanded magnitude' and space concept.
So what's the commonality here? I believe when Riemann is considering a 'multiply extended magnitude', he's thinking of a vector of the appropriate dimension, a 'position' in a space. So a 1 dimensional line becomes <x>, ranging from -1 to 1 draws the usual section of the number line between [-1,1], a 2 dimensional area becomes characterised in the form <x,y>, with constraints on <x,y> to specify the area (eg x^2+y^2<=1 for a circle centred at the origin with radius 1) or <x,y,z> to specify a volume (with x^2+y^2+z^2<=1 for a sphere centred at the origin with radius 1). (Edit: though it's worthwhile noting here that 'coordinate system' is maybe a better representation of the concept, but the distinction between vector space and coordinate system probably doesn't matter at this point in the exegesis, in which the concepts are fuzzy) The idea of a 'multiply extended' magnitude is just that of a collection of 1 dimensional magnitudes.
Note at this point we have a sense for the 'size' of 1 dimensional, 2 dimensional and 3 dimensional magnitudes - length, area, volume-, and we also have multiply extended magnitudes being a collection of independently varying 1 dimensional magnitudes (the x and y directions in the plane, say, are both 1 dimensional magnitudes which together form a 2 dimensional magnitude). So Riemann sets himself the task of:
I have in the first place, therefore, set myself the task of constructing the notion of a multiply extended magnitude out of general notions of magnitude.
defining/mathematically characterising/axiomatising notions of size (like length, area, volume) for multiply extended magnitudes (like lines, circles, spheres).
But it is worthwhile to note that Riemann is explicitly considering
notions of space, so we're considering things 'one layer back' from lines, circles, spheres - we're considering ways of linking
geometries to
sizes. The first example of which in the paper is trying to construct/axiomatise the usual notion of length/area/volume in Euclidean space. So when Riemann says:
It will follow from this that a multiply extended magnitude is capable of different measure-relations, and consequently that space is only a particular case of a triply extended magnitude.
he's talking about the fact that completely characterising, say, the relationship between space and volumes mathematically - you can change this relationship in accord with some notion end up with an inequivalent notion of space. This drives a 'hard wedge' as it were between the
necessity of the relationship between (1)
the space intuition and (2)
its complete axiomatisation; there is now more than one space intuition/notion, revealed by the ability to modify axioms/characterisations of space. Shifting vocabularies, there's no unique mathematical 'space intuition' a priori, since we can characterise others - and perhaps, tentatively, this means the reason for the darkness between (1) and (2) is an
elision inherent in previous geometric thought generated by the belief that studying space intuitions always meant articulating a single a priori notion of space (eg Euclidean space, that which is described by Euclid in his Elements). Because of this
hence as a necessary consequence that the propositions of geometry cannot be derived from general notions of magnitude
(because of the plurality of magnitude notions revealed by Riemann's approach) and thus:
the properties which distinguish space from other conceivable triply extended magnitudes are only to be deduced from experience.
we must recognise what space-like notion is appropriate for whatever purposes we may have. Riemann then seeks to find indicators - necessary and sufficient conditions / characterisations - of notions of space (and multiply extended magnitudes more generally) - of which space concept is appropriate for which purpose.
Thus arises the problem, to discover the simplest matters of fact from which the measure-relations of space may be determined; a problem which from the nature of the case is not completely determinate, since there may be several systems of matters of fact which suffice to determine the measure-relations of space - the most important system for our present purpose being that which Euclid has laid down as a foundation.
and moreover the existence of multiple n-dimensional magnitude concepts (like the link between 2 dimensional spaces and areas) severs the a priori connection between Euclidean space(s) and space, as n dimensional magnitude, simpliciter.
One illustrative example here is that for distances on the surface of the Earth, if they're short we can use Euclidean geometry to calculate them, but if they're long we can't - the surface of a sphere is not Euclidean, it wraps around itself, it has curvature and so on.
Thus, the a priori necessity of space being Euclidean space, or more generally of space being uniquely characterised, is broken by the plurality of n dimensional magnitudes and measures of their length/area/volume. In essence, Riemann is playing a game of constructing counterexamples to Euclidean space after characterising precisely what it is! Find the boundaries of the concept, find the exceptions, and vice versa.
Because we no longer have the a priori necessity of our calculations about space, destroyed by the non-uniqueness of space concepts, this renders which space concepts nature can be modelled by as a matter of investigation:
These matters of fact are - like all matters of fact - not necessary, but only of empirical certainty; they are hypotheses. We may therefore investigate their probability, which within the limits of observation is of course very great, and inquire about the justice of their extension beyond the limits of observation, on the side both of the infinitely great and of the infinitely small.
and of purely mathematical consequences/assumptions of them ('beyond the limits of observation').
The relationship to infinitely great and infinitely small probably connotes the fact that Riemann will be studying space at multiple scales; the geometry relationship between 2 dimensions and volumes, say, becomes defined with respect to infinitely small variations (like dx and dy in calculus), and it may be that on larger scales different mathematical patterns can hold even within the same notion of space (like my sphere example above).
Edit: note that when I'm using <> to surround something, that's notation that refers to a coordinate system being in play. So EG <x> denotes a position on (something like/for example) the real line, <x,y> denotes a position in in the plane (or something like it/for example) and so on.