In practical terms, this meant that for a ship in hyper, the distance between normal-space points was "shorter," which allowed the vessel to move between them using a standard reaction drive at sublight speeds to attain an effective FTL capability. Even in hyper, ships were not capable of true faster-than-light movement; the relatively closer proximity of points in normal-space simply gave the appearance of FTL travel, which meant that as long as a vessel was dependent on its reaction drive and could not reach the higher hyper bands, its maximum apparent speed was limited to approximately sixty-two times that which the same vessel could have attained in normal-space.
Navigation, communication, and observation all are rendered difficult by the nature of hyper-space. Formed by gravitational distortion, hyper-space itself acts as a focusing glass, producing a cascade effect of ever more tightly warped space. The laws of relativistic physics apply at any given point in that space, but as a hypothetical observer looks "outward" in hyper-space, his instruments show a rapidly increasing distortion. At ranges above about 20 LM (359,751,000 km.) that distortion becomes so pronounced that accurate observations are impossible. One says "about 20 LM" because, depending on local conditions, that range may vary up or down by as much as 12% — that is, from 17.6 LM (316,580,880 km.) to 22.4 LM (or 402,921,120 km.). A hypership thus travels at the center of a bubble of observation from 633,161,760 to 805,842,240 km. in diameter. Even within that sphere, observations and measurements can be highly suspect; in effect, the "bubble" may be thought of as the region in which an observer can tell something is out there and very roughly where. Exact, precise observations and measurements are all but impossible above ranges of 5,000,000 to 6,000,000 km., which would make navigational fixes impossible even if there were anything to take fixes on.
This seemed to rule out any practical use of hyper-space until the development of the first "hyper log" (known as the "HL" by spacers) in 731 pd. The HL is analogous to the inertial guidance units first developed on Old Earth in the 20th century ce. By combining the input from extremely acute sensor systems with known power inputs to a vessel's own propulsive systems and running a continuous back plot of gravity gradients passed through, the HL maintains a real-time "dead reckoning" position. Early HLs were accurate to within no more than 10 LS per light-month, which meant that, in a voyage of 60 light-years, the HL position might be out by as much as two light-hours. Early hyper-space navigators thus had to be extremely cautious and make generous allowances for error in plotting their voyages, but current (1900 pd) HLs are accurate to within .4 light-second per light-month (that is, the HL position at the end of a 60 light-year voyage would be off by no more than 288 light-seconds or less than 5 light-minutes).
From the beginning of hyper travel, it was known that there were multiple hyper bands and that the "higher" the band, the closer the congruity between points in normal-space and thus the higher the apparent FTL speed, but their use was impractical for two major reasons. First, translation from band to band bleeds off velocity much as the initial translation. The bleed-off for each higher band is approximately 92% of the bleed-off for the next lowest one (that is, the alpha band translation reduces velocity by 92%; the beta band bleed-off is 84.64%; the velocity loss for the gamma band is 77.87%, etc.), but it still had to be made up again after each translation, and this posed an insurmountable mass requirement for any reaction drive.
The second problem was that the interfaces between any two hyper bands are regions of highly unstable and powerful energy flows, creating the "dimensional shear" which had destroyed so many early hyperships, and dimensional shear becomes more violent as band levels increase. Moreover, even the relatively "safe" lower bands which could be reliably reached were characterized by powerful energy surges and flows — currents, almost — of highly-charged particles and warped gravity waves. Adequate shielding could hold the radiation effects in check, but a grav shear within any band could rip the strongest ship to pieces.
Hyper-space grav waves take the form of wide, deep volumes of space, as much as fifty light-years across and averaging half their width in depth, of focused gravitational stress "moving" through hyper-space. Actually, the wave itself might be thought of as stationary, but energy and charged particles trapped in its influence are driven along it at light— or near-light-speed. In that sense, the grav wave serves as a carrier for other energies and remains motionless but for a (relatively) slow side-slipping or drifting. In large part, it is this grav wave drift which makes them so dangerous; survey ships with modern sensors can plot them quite accurately, but they may not be in the same place when the next ship happens along. The major waves in the more heavily traveled portions of the galaxy have been charted with reasonable accuracy, for sufficient observational data has been amassed to predict their usual drift patterns. In addition, most waves are considered "locked," meaning that their rate of shift is low and that they maintain effectively fixed relationships with other "locked" waves. But there are also waves which are not locked — whose patterns (if, in fact, they have patterns at all) are not only not understood but can change with blinding speed. One of the most famous of these is the Selkir Shear between the Andermani Empire and the Silesian Confederacy, but there are many others, and those in less well-traveled (and thus less well-surveyed) areas, especially, can be extremely treacherous.
The heart of any grav wave is far more powerful than its fringes, or, put another way, a "grav wave" consists of many layers of "grav eddies." For the most part, all aspects of the wave have the same basic orientation, but it is possible for a wave to include counter-layers of reverse "flow" at unpredictable vertical levels. Despite the size of a grav wave, most of hyper-space is free of them; the real monsters that are more than ten or fifteen light-years wide are rare, and even in hyper the distances between them are vast, though the average interval between grav waves becomes progressively shorter as one translates higher into the hyper bands. The great danger of grav waves to early-generation hyperships lay in the phenomenon known as "grav shear." This is experienced as a vessel moves into the area of influence of a grav wave and, even more strongly, in areas in which two or more grav waves impact upon one another. At those points, the gravitational force exerted on one portion of the vessel's structure might be hundreds or even thousands of times as great as that exerted on the remainder of its fabric, with catastrophic consequences for any ship ever built.
In theory, a ship could so align itself as to "slide" into the grav wave at an extremely gradual angle, avoiding the sudden, cataclysmic shear which would otherwise tear it apart. In practice, the only way to avoid the destructive shearing effect was to avoid grav waves altogether, yet that was well nigh impossible. Grav waves might be widely spaced, but it was impossible to detect them at all until a ship was directly on top of one, and with no way to see one coming, there was no way to plot a course to avoid it. It was possible to recognize when one actually entered the periphery of a grav wave, and if one were on exactly the right vector, prompt emergency evasion gave one a chance (though not a good one) of surviving the encounter, but the grav wave remained the most feared and fearsome peril of hyper travel.