Four Lectures on Relativity and Space Visual Map
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Section titled “Modern Guide Diagrams Keyed To This Source”Field Of Energy Boundary
Modern reading aid for Steinmetz’s field language in Relativity and Space.
field-language, ether, relativity, energy-field
Candidate Figure References
Section titled “Candidate Figure References”| Candidate | Caption lead | Section | Routes |
|---|---|---|---|
four-lectures-relativity-space-fig-002Fig. 2 | M Fig. 2. 18 RELATIVITY AND SPACE | Lecture 2: Conclusions From The Relativity Theory | source research review |
four-lectures-relativity-space-fig-004Fig. 4 | M Fig. 4. 22 RELATIVITY AND SPACE | Lecture 2: Conclusions From The Relativity Theory | source research review |
four-lectures-relativity-space-fig-005Fig. 5 | none returned to the radiator. Fig. 5. CONCLUSIONS FROM RELATIVITY THEORY 23 | Lecture 2: Conclusions From The Relativity Theory | source research review |
four-lectures-relativity-space-fig-006Fig. 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 research review |
four-lectures-relativity-space-fig-008Fig. 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 research review |
four-lectures-relativity-space-fig-009Fig. 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 research review |
four-lectures-relativity-space-fig-010Fig. 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 research review |
four-lectures-relativity-space-fig-014Fig. 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 research review |
four-lectures-relativity-space-fig-015Fig. 15 | 7 ’ Fig. 15. standing near the track, shoot a rifle bullet through the car, | Lecture 3: Gravitation And The Gravitational Fleld | source research review |
four-lectures-relativity-space-fig-016Fig. 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 research review |
four-lectures-relativity-space-fig-017Fig. 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 research review |
four-lectures-relativity-space-fig-020Fig. 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 research review |
four-lectures-relativity-space-fig-021Fig. 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 research review |
four-lectures-relativity-space-fig-025Fig. 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 research review |
four-lectures-relativity-space-fig-029Fig. 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 research review |
four-lectures-relativity-space-fig-030Fig. 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 research review |
four-lectures-relativity-space-fig-031Fig. 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 research review |
four-lectures-relativity-space-fig-032Fig. 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 research review |
four-lectures-relativity-space-fig-033Fig. 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 research review |