Four Lectures on Relativity and Space Visual Map

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Field Of Energy Boundary

Modern reading aid for Steinmetz’s field language in Relativity and Space.

field-language, ether, relativity, energy-field

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Candidate Figure References

Candidate	Caption lead	Section	Routes
four-lectures-relativity-space-fig-002 Fig. 2	M Fig. 2. 18 RELATIVITY AND SPACE	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-004 Fig. 4	M Fig. 4. 22 RELATIVITY AND SPACE	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-005 Fig. 5	none returned to the radiator. Fig. 5. CONCLUSIONS FROM RELATIVITY THEORY 23	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-006 Fig. 6	•^W///y/y/y/////////////‘//vy/////////’//^/^^////^>>^ Fig. 6. hour, relative to the track B. Let us denote the distance relative to the train — that is, measured in the train^ — ^by	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-008 Fig. 8	and (2), are very similar to those representing a rotation of Fig. 8. the coordinate axes by an angle tan co = v/c. If it were such	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-009 Fig. 9	r 7’ Fig. 9. P1P3’ is not the time but a combination of time and length. Inversely, to the second observer P1P3’ is the time and	Lecture 2: Conclusions From The Relativity Theory	source workbench
four-lectures-relativity-space-fig-010 Fig. 10	R = M. Fig. 10. Let (in Fig. 10) 5 be a body revolving around a point 0. The fundamental law of physics is the law of inertia.	Lecture 3: Gravitation And The Gravitational Fleld	source workbench
four-lectures-relativity-space-fig-014 Fig. 14	<^-<-r) B Fig. 14. constant speed in a straight line, but curves backward, just as it did in Fig. 13 on a 10 per cent up grade at constant	Lecture 3: Gravitation And The Gravitational Fleld	source workbench
four-lectures-relativity-space-fig-015 Fig. 15	7 ’ Fig. 15. standing near the track, shoot a rifle bullet through the car,	Lecture 3: Gravitation And The Gravitational Fleld	source workbench
four-lectures-relativity-space-fig-016 Fig. 16	>Vf Fig. 16. leaves the car, at the point B of the track, it is greater and is v^. Then the angle which the bullet makes relative	Lecture 3: Gravitation And The Gravitational Fleld	source workbench
four-lectures-relativity-space-fig-017 Fig. 17	until finally, at the extremely high velocity of light, c = Fig. 17. 186,000 miles per second, the hyperbola (6) becomes almost a straight line. Even if the beam of light comes very close	Lecture 3: Gravitation And The Gravitational Fleld	source workbench
four-lectures-relativity-space-fig-020 Fig. 20	R = j/VK. (15) Fig. 20. E. THE STRAIGHT LINE AND THE ELLIPTIC 2-SPACE	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-021 Fig. 21	line between them, as Li or L2 — shown dotted in Fig. 21 — Fig. 21. is longer. Suppose we have a straight line L in the plane Fig. 21 and a point P outside of L. Any line drawn in the	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-025 Fig. 25	The mathematical n-space merely is the continuous mani- FiG. 25. fold of oo« elements which are given by the n ratios: x : y :	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-029 Fig. 29	however, are no part of projective geometry, as they are Fig. 29. made by its relation to infinity and therefore are metric in character : The hyperbola has two infinitely distant points,	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-030 Fig. 30	with regard to a conic, then the line connecting the points Fig. 30. pi and P2 is the polar of the point of intersection of Pi and	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-031 Fig. 31	of these six lines by e = ah, cd;f = ac, hd; g = ad, he, and Fig. 31. draw the three additional lines ef, eg and fg, we get a total of nine lines and four points on each of these nine lines.	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-032 Fig. 32	tant (that is, very far distant) we thus recognize by the Fig. 32. two lines of sight from our eyes to the object having the same direction.	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench
four-lectures-relativity-space-fig-033 Fig. 33	parallels Li and Lo through a point P — that is, two lines Fig. 33. which intersect L at infinity — and these tvv^o parallels Li and L2 make an angle L1PL2 with each other. Thus L]	Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field	source workbench