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Diagnostic ultrasound ( PDFDrive )

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490 PART II Abdominal and Pelvic Sonography

localized along the craniocaudal axis. Although diastasis usually

does not, epigastric hernias oten do cause tenderness.

Epigastric linea alba hernias are easier to diagnose than are

groin hernias as long as they are scanned with the proper

transducer and the sonographer or physician is actually visually

inspecting the linea alba. Epigastric hernias are usually supericial

enough in location that they are best shown with 10- to 12-MHz

linear array transducers. With these transducers, the defect

through the linea alba is usually quite conspicuous because it is

either isoechoic or hypoechoic compared with the extremely

hyperechoic linea alba. he defect is usually very near the midline,

but it may occur eccentrically toward the right or let side of the

linea alba (see Fig. 13.39D-E; Figs. 13.41 and 13.42, Video 13.14).

he most frequent reason for missing an epigastric linea alba

hernia is that the examination for abdominal pain was performed

with the standard 3-MHz curved linear array transducer, focused

too deep in the elevation axis to identify any structures except

large hernias in obese patients. he clinician must have an index

of suspicion to use the appropriate transducer.

Although clinically detected epigastric hernias tend to be quite

large and oten contain bowel and other intraperitoneal contents,

sonographically detected epigastric hernias are usually small to

moderate-sized and contain only preperitoneal fat (Video 13.15).

In hernias that contain only preperitoneal fat, the underlying

peritoneal membrane and transversalis fascia are intact and the

hernia cannot be seen or repaired laparoscopically. Epigastric

hernias always have a very narrow neck in comparison to the

size of the fundus and thus are usually not reducible and are at

increased risk for strangulation, even when small. Some epigastric

hernias that contain only preperitoneal fat are so small that it is

diicult to believe that herniation is the cause of pain (Fig. 13.43).

hese hernias are not palpable, and patients typically have pain,

which more likely results from the tear or tendinosis of the linea

alba than from herniation of a tiny amount of properitoneal fat.

A B C

FIG. 13.41 Epigastric Linea Alba Hernia. Mesenteric fat protrudes through a 1-cm defect (calipers) in the linea alba at midline just above the

umbilicus. Images were obtained in the transverse supine (A), transverse with patient sitting (B), and sagittal with patient sitting (C). Note the

change in the appearance of the hernia defect with change in patient position.

A

B

FIG. 13.42 Large Ventral Hernia. Large fat-containing hernia is visible just left of midline. (A) and (B) Transverse images show the hernia in

the region of patient’s pain in palpable abnormality. See also Video 13.14.

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